When Dead Stars Collide

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Before the first stars were born, the Universe was an expanse of featureless darkness – devoid of light and life. The first generation of stars to shatter this swath of blackness, with their fierce stellar fires, were not like the stars we see today, because they were not born the same way. The first stars were giants, that formed directly from the lightest of all atomic gases – mostly hydrogen, with a smaller amount of helium, both of which formed in the wildly expanding fireball of the Universe's mysterious Big Bang birth nearly 14 billion years ago. The first stars are responsible for changing the Universe from what it was then, to what it now is. This is because they created, in their nuclear-fusing hearts, all of the atomic elements heavier than helium, so "polluting" the cosmos with the atomic elements that made planets, moons, and people possible. In June 2018, scientists at the California Institute of Technology (Caltech) in Pasadena, announced that they have found, for the first time, that colliding and merging duos of denut neutron stars are responsible for creating the most heavy atomic elements present in small dwarf galaxies , shedding new light on yet another mystery of star-birth.

Heavy atomic elements, such as gold and silver, are called "metals" by astronomers, and they are of critical importance for planet formation, as well as the emergence of life itself. By observing these relatively tiny dwarf galaxies , the scientists hope to learn more about the primary sources of "metals" for the universe.

The origin of most of the heaviest atomic elements listed in the familiar Periodical Table, including 95% of all the gold present on Earth, has been a subject of debate among astronomers for decades. However, it is now understood that the heavy "metals" are created when the nuclei of atoms within stars snare elementary particles called neutrons. In the case of most elderly stars, including those inhabiting the dwarf galaxies observed in this study, the process happens very quickly – and, as a result, is termed an r-process , where the r signifies "rapid."

There are currently two proposed potential sites where the r-process is theorized to take place. The first possible site is a rare form of supernova called a magnetorotational supernova, which is a type of stellar explosion that can create large magnetic fields. The second proposed site involves two neutron stars that collide and then merge. In August 2017, the National Science Foundation (NSF) -funded Interferometry Gravitational-wave Observatory (LIGO) , along with other ground-based telescopes, spotted just such a neutron star collision that was in the middle of creating a treasure trove composed of the heaviest atomic elements. However, observing only one event is not sufficient to tell astronomers where most of these heavy "metals" are created within galaxies.

Stellar Generations

Astronomers classify stars as either Population I (metal-rich) or Population II (metal-poor). However, even the most metal-poor stars belonging to Population II contain small amounts of metals. This means that these metal-poor ancient stars are composed of more than just the pristine hydrogen and helium gas that was produced in the Big Bang (Big Bang Nucleosynthesis) . For this reason, there had to exist an earlier population of stars to manufacture these heavy metals.

Therefore, astronomers were forced to suggest the existence of a third stellar population – the very ancient Population III stars that were composed entirely of ancient primordial gas that had been churned out in the Big Bang. Big Bang Nucleosynthesis produced only hydrogen, helium, and trace quantities of lithium or beryllium. The first stars produced the first batch of metals that "polluted" younger generations of stars. Population III stars served as the source of the small amount of metals observed in the metal-poor Population II stars.

The more massive the star, the shorter its hydrogen burning "life." Massive stars burn their necessary supply of nuclear-fusing hydrogen fuel in their cores much more rapidly than smaller stars, thus manufacturing increasingly heavier and heavier atmospheric elements out of lighter ones. The end comes when the massive star finally has managed to fuse for itself a core of iron that can not be used for fuel. At this terrible grand finale of a massive star's "life", it collapses and then blows itself to smithereens in a fatal supernova blast. In contrast, relatively small stars like our Sun – which is a metal-rich Population I star – blissfully burn their hydrogen fuel for about 10 billion years. More massive stars, however, "live" for mere millions, as opposed to billions, of years and do not die quietly. When small stars like our Sun reach the end of the stellar road they first become swollen Red Giant stars that historically puff off their outer gaseous layers. The relic core of a small Sun-like star becomes a dread dead stellar corpse, called a white dwarf , that is surrounded by a beautiful, multicolored, sparkling shroud of what was once the dead progenitor star's outer gases.

Therefore, massive stars, like Population III stars – as well as younger generations of massive stars – do not die in peace. They go out with a bang. When a massive star dies, it explodes as a supernova – a brilliant fatal blast that causes the erstwhile star to either leave a relic neutron star behind, or a stellar mass black hole. The core-collapse (Type II) supernova blasts out into space a good-bye gift to the Universe – its freshly forged batch of metals . These metals will absolutely be incorporated into Populations I and II stars – with all of their beautiful life-sustaining possibilities. We are here because the stars are here.

Stellar Burn-Out

Neutron stars are both the smallest and densest of known stellar objects. Usually, a neutron star will sport a radius of about 6.2 miles and a mass that ranges between 1.4 and 3 times that of our Sun. They are the end-product of a supernova that has compressed the core of the massive progenitor star to the density of an atomic nucleus. Once born, neutron stars can no longer generate heat, and they cool off as time goes by – but, it is still possible for them to evolve further as a result of collisions or accretion.

Most models indicate that neutron stars are almost entirely made up of neutrons , which are subatomic particles with no net electrical charge and with a slightly larger mass than protons. Protons and neutrons form the nuclei of atoms. Electrons and protons present in normal atomic matter combine to create neutrons at the conditions of neutron stars.

Neutron stars that have been observed are extremely hot, with a surface temperature of approximately 600,000 Kelvin. They are so incredibly weak that a teaspoon full of neutron star stuff would have a mass of about 3 billion tons. Their magnetic fields are between 100 million to 1 quadrillion times as powerful as that of our planet. The gravitational field at a neutron star 's surface is about 200 billion times that of Earth.

As the massive progenitor star's core collapses, its rotation rate increases due to the conservation of angular momentum. As a result, newborn neutron stars spin at up to several hundred times per second. Some neutron stars emit regular beams of electromagnetic radiation that make them detectable as pulsars. Indeed, these emitted beams are so extremely regular that they are frequently compared to lighthouse beacons on Earth. The 1967 discovery of pulsars by Dr. Jocelyn Bell Burnell provided the first observational evidence that neutron stars really exist in nature.

Astronomers think that there are approximately 100 million neutron stars inhabiting our Milky Way Galaxy. This number has been obtained by scientists calculating the number of stars that have gone supernova in our Galaxy. However, even though the neutron stars that have been observed so far are searing-hot, most neutron stars are old, cold, and difficult to find – unless they are in their neonatal pulsar stage or are members of a tattle-tale binary system . Lazily-rotating and non-accreting neutron stars are almost undetectable. However, thanks to the highly successful Hubble Space Telescope, some neutron stars that apparently emit only thermal radiation have been spotted. Neutron stars in binary systems can experience accretion which makes the system bright in X-rays while the material is tumbling onto the neutron star , thus forming hotspots that rotate in and out of view in identified X-ray pulsar systems. Such accretion can "rejuvenate" older pulsars and potentially cause them acquire more mass and spin-up to extremely rapid rotation rates, so forming what are termed millisecond pulsars . These binaries will continue to evolve, and quite the companion stars can also become compact stellar relics, such as white dwarfs and neutron stars themselves – although some other possibilities include the total destruction of the luckless companion through either merger or ablation. The merge of binary neutron stars may be the source of what are called short-duration gamma-ray bursts – the strong sources of ripples in Spacetime termed gravitational waves. In 2017, just such a direct detection of gravitational waves from this type of event was made, and gravitational waves have also been indirectly spotted in a system where a duo of neutron stars orbit each other.

When Burnt-Out Stars Collide

The team of Caltech astronomers studied several dwarf galaxies in order to observe the production of atomic elements in galaxies as a whole. For this purpose, the researchers used the WM Keck Observatory in Maunakea, Hawaii. Our own Milky Way, although quite large, is generally considered to be about average in size – at least, as far as galaxies go. However, these relatively tiny dwarf galaxies , which are in orbit around our Milky Way, contain a puny 100,000 times less mass in stars than our Galaxy. The astronomers were on the hunt for when the heaviest metals in the small galaxies were made. This is because m agnetorotational supernovae tend to occur in the ancient Universe, while neutron star mice happened later in the Universe's history.

The results of the Caltech study, submitted for publication in The Astrophysical Journal , were presented at the 232nd meeting of the American Astronomical Society (AAS) held in June 2018 in Denver, Colorado. The Caltech astronomers' study provides evidence that the main sources of the r-process in dwarf galaxies occur over the passage of a reliably long timescale. This means that the heavy atomic elements were manufactured later in the history of element production in galaxies. By measuring the ratio of elements in stars of varying ages, the scientists were able to say when these elements were created in our Milky Way.

"This study is based on the concept of galactic archaeology, which uses the elements present in stars today to 'dig up' evidence of the history of element production in galaxies. able to say when these elements were created in the Galaxy, "Dr. Evan Kirby explained to the press on June 5, 2018. Dr. Kirby is an assistant professor of astronomy at Caltech.

Astronomers frequently study dwarf galaxie s as a method of learning about galaxies in general. Because these galaxies are relatively small, they possess less complicated histories that are easier to read than those of their larger galactic kin.

Gina Duggan, a Caltech graduate student and lead author of the new research, commented that "Unlike the Milky Way, which has attracted stars from other galaxies through its history, these dwarf galaxies were isolated when their stars were born, allowing galactic archaeology to clearly track the buildup of r-process elements over time. This provides an important clue for the timescale of the dominant source of r-process production across the Universe for the first time. "

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Source by Judith E Braffman-Miller

Grundig DTR 3000 Table Digital Radio, 30 W PMPO, AUX-IN, UKW-RDS und DAB+ mit jeweils 10 Stationsspeicher schwarz

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Hair Loss Treatment With Lasers

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We've all heard about the marvels of lasers, from the technological breakthroughs in laser surgery to whitening teeth. But did you know that there have been breakthroughs using lasers as a hair loss treatment using low-light lasers? In fact, the technology behind lasers as a hair loss treatment, also called "laser hair regrowth therapy" has been around for more than twenty years, and has been used extensively in Europe successfully treating hair loss. Only in the past decade have low-light lasers come into widespread use in laser hair regrowth therapy here in the Unites States. Hand-held laser devices have recently been approved by the FDA as a hair loss treatment, giving it a new credibility it has long enjoyed in Europe.

While studies show that some 90% of clients who use laser hair regrowth therapy as a hair loss treatment method see a marked change in the quality of their hair, its thickness and its shedding, there's more to the story than that. A reputable hair treatment clinic will tell you what many other clinics will not tell you: that hair loss is a complex issue and your results will vary depending on the care you get. If you choose a treatment like laser hair regrowth therapy, you will want to visit a reputable practitioner for best results that will address your individual hair loss situation.

So what are the top five things you should know when looking into laser hair regrowth therapy?

o When choosing a hair loss treatment, seek out a multi-therapeutic approach – While steady and effective laser hair regrowth therapy will make a difference in your hair, your best results will be seen using a multi-therapeutic approach. What does that mean? It means taking advantage of all the technology out there. What we know is that the major cause of male and female pattern baldness is the excess of something called DHT (Dihydrotestosterone) in the scalp. DHT effectively cuts off the nutrition of a hair follicle (oxygen, blood supply, nutrients.) With laser hair regrowth therapy the low-light laser penetrates this level of the skin and allows a richer blood flow to reach the hair follicle . But used in conjuction with a hair loss treatment such as DHT inhibitors like Rogaine, Propecia and / or Minoxidil with 5% saw palmetto can greatly improve the quality of the hair loss treatment. Products like these help to stop shedding in its tracks, giving the laser hair regrowth therapy a chance to work. Also, shampoos that inhibit DHT with products like saw palmetto and other DHT-blocking herbs promote a healthy scalp can improve circulation and overall effectiveness of laser hair regrowth therapy.

o Length of Treatment – Contrary to popular myth, use of laser hair regrowth therapy is not a one-stop shopping experience. It's a long-term hair loss treatment; a real commitment and results will not begin to be seen until a client has been using the clinic's low light laser for at least three months. That's partly due to the hair's life cycle. As new hair begins to emerge, it comes in thicker and stronger. But most successful clients make a commitment of between 1-2 years of office visits and then maintain their new, healthy hair with a hand-held home laser, an important and inexpensive part of the hair loss treatment.

o With laser hair regrowth therapy, the more diodes the better – Diodes are the little points of light emitted by a low-light laser. In a typical clinic low-light laser, there are diodes placed strategically in the curved surface of the machine that can treat the entire scalp at once. But make sure you look for the number of diodes your machine has. The more diodes, the better (more effectively) the laser will work. This is why, for laser hair regrowth therapy, hand-held lasers (which use few diodes) are preferred for maintenance, not the initial hair loss treatment.

o Consult an expert in laser hair regrowth therapy – There are many less-than-legit treatment clinics opening up, claiming to know the business. Anyone can purchase a low light laser and call itself an expert. But an expert clinician will employ both doctors specializing in treatment, and knowledgeable consultants on their teams. When you decide to look into laser hair regrowth therapy, be sure to check the pedigree of the clinic you're visiting. The laser hair loss experts you are seeking have been in business for a long time and have great reputations that are easily researched online. Experts at these treatment clinics can tell you exactly what you need and what will and will not work for your particular hair loss condition. Do not set for less than the best.

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Source by Ray Treadwell

Amazon.de Geschenkkarte in Grußkarte – 30 EUR (Glückwunsch Sterne)

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Gültigkeit der Gutscheine beträgt zehn Jahre ab Kauf.
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Blue Man Group Tickets – True Blue Wonders

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Blue Man Group Continues to Delight Audiences

Live performances can dazzle audiences when what they are seeing is uniquely different. One of the most innovative and uniquely different acts now seen on tours as well as in Vegas is the Blue Man Group, a trio of androgynous beings that are quite literally…Blue. This group was created in 1988 and is listed under the genre of performance art and music, but truly, there is no one clear way to define the BMG. In the 20 years since the group’s inception, they have delighted and amazed audiences of all ages and their newest live shows are continuing to win them many more admiring fans. The best Blue Man Group Tickets are quickly claimed within the first few days of being offered which is a very strong indicator of just how popular this trio really is.

Understanding the Performers

The Blue Man Group does not speak or utter any sounds during their performances, but they always communicate perfectly with their audience and each other. Their unique communication is established through eye contact, subtle but well rehearsed hand and head movements, and other choreographed body language. The trio is so expert at this type of silent interaction that they can convey emotions of curious wonder, surprise or delight without resorting to overly exaggerated motions. Audiences delight in the uniform look of the group members with their earless, hairless, neon blue heads and identical appearances. Although the main trio generally performs in harmony, there are some hilarious skits that involve one of the three being just slightly out of sync with the others.

The Blue Man Group Performances – Made For Fun

There are always pictures, words, instructions, or information that is being flashed on screens behind the performers. These vary at each show but sometimes the screen shots simply show some funny messages using the real names of ticket holders. You might also witness some ditzy slogans, cute pictures, photos from the current newspapers or even candid shots of people in the audience. This is done to entertain and provide diversion while you are waiting for the show to begin. All of this pre-show activity is interesting and most is undeniably hilarious, especially if your name (or some you recognize) makes it onto the montage.

As the show revs into gear, there are frequently important announcements and instructions that are flashed on the giant screen located behind the performers. Although the words are large and clearly printed, there is always an unseen narrator that reads them aloud for you. Using this compelling off stage voice is a great way to gently encourage the audience to follow the instructions that are flashing. This interactive stage performance is one of the few live shows that really make a connection with everyone in the audience. Whether you become a fist pumping rock star in training or a poncho covered art critic ducking spurting drumbeats of colorful paint the Blue Man Group will make sure that you have the time of your life.

The group incorporates different themes for their shows, and some of these are information overload, innocence, and imitation. The theme of imitation is used during their How to Be a Rock Star show that offer instructions on how you can metamorphose into a rocker. There is an unseen narrator that will read the instructions as they are flashed onto the screen and he is able to compel people to get involved early. This program gets everyone out of their seats and moving.

Soon the audience is filled with people of all ages who are performing fist pumps, and exaggerated dance movements. Instruction is always available because the Blue Man Group is performing the same moves on stage. However, there is a very cool animated stick figure on screen to show you the moves as well. For sheer party fun, this is one of the most popular shows that fans come to see.

The Blue Man Group – Keeping it „Real Fun“

Toilet paper, crepe paper, balloons, and truly weird musical instruments are also a major part of any of the BMG events, and if you have Blue Man Tickets for seats in the front rows don’t forget your ponchos. The group already has a schedule that includes US, Canadian and worldwide tours in addition to their current Las Vegas run. This keeps the group working at a frantic level and even with more than 500 BMG performers, they are pressed to keep up with the demand for performances.

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Source by Matt Joal

Aigle Lolly Pop Print Gummistiefel, Unisex-Kinder Gummistiefel, Mehrfarbig (marine/etoile N), 28 EU (10 UK)

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Weite: Mittel
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How to Ollie Fast – How to Ollie in Two Weeks or Less

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The ollie is one of the easiest skateboarding tricks, yet one of the most important. Learning how to do an ollie can seem like a challenging task to beginner skateboarders, but if set and follow a two week action plan, you’re guaranteed to learn how to ollie in no time!

I strongly recommend that you practice from half an hour to an hour a day if you want to learn how to ollie as quick as you can. I suggest you practice on weekdays and take a break or just go skate around on the weekends.

Before you start, you must know what the ollie looks like. I suggest you watch some „how to ollie“ videos on the internet so you know how they should look and the basic steps.

Days 1-2

For the first two days, you’ll want to practice getting the foot position down. Footing is key in learning how to ollie!

You want to place your front foot a little ahead of the board, and your back foot on the tail of the skateboard, with the ball of your back foot in the center of the tail. For the first two days, just practice this foot position and make sure you’re comfortable.

Days 3-5

For the rest of the week, I recommend you practice the general motion of the ollie. One of the most helpful ways to learn how to ollie is to visualize the trick in your mind first.

Stand over the board, in the ollie position. See yourself:

1. Popping the tail by slamming your back foot down hard on the tail

2. Jumping up

3. Dragging your front foot up towards the front of the board and

4. Leveling the board out and landing on the skateboard bolts

The key in learning how to do an ollie is being able to put those three things together.

After you visualized the ollie, it’s time to stand on the board and try it out. Remember to slam, jump, and drag.

Days 8-14

For the second week, you should continue practicing your ollies. By now, you should know exactly how to do an ollie, but probably have trouble actually getting the skateboard up. If you’re having a little bit of trouble, try out these tips:

– Do not bend too far down, because this can throw off your balance. Just give a slight squat.

– Suck up your legs after you pop to help get the board in the air

– Stay centered over your board as you pop and aim to land over the bolts

The only way to overcome this is practice and persistence. You have to experiment with the timing of the trick until you find something that works for you. It took me more than a month before I learned how to ollie.

Congratulate yourself when you finally learn how to ollie. You can now take them to new places, such as onto curbs, off of ledges and over obstacles!

Good luck learning how to ollie!

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Source by Mark Weth

Classic Pet Products Katzenminze Schläger und Ball

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Text Message Market – 5 Benefits For Restaurants

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Restaurant marketing is a complex issue. There are so many ways to promote these days: Text advertising, print media, social media, word of mouth and many others. Here are some benefits of text message advertising to help you choose.

1. Generates repeat business from existing customers

You will be advertising to customers that have asked to receive your messages. One goal of text advertising is to get existing customers to visit you more frequently. By offering them updates and text coupons you can remind customers of events and ask them to come enjoy a special offer.

2. Bring customers through the door on slow days

Like any business you have days that are slower then you like. Text message advertising allows you to send immediate offers to your customers when you need them to come in. No other advertising provides this kind of immediate response.

3. Attract new customers

Encourage your opted-in patrons to share your offers with friends. Text coupons can be forwarded from phone to phone; so go viral, make an offer worth sharing and get friends of your customers to come through the door with a special offer. have them opt-in to your text campaign and grow your list for future ads.

4. Measure the effectiveness of other ads

Are you spending money on print, radio or TV ads? You can put a keyword response into each ad to measure how many potential customers those ads are creating for you. If you see that certain ads have little response, cut them from your budget and save yourself some money.

5. Engage your customers

Utilizing Text-To-Win and Text-To-Vote campaigns can be a fun way to interact with customers. Learn what they like and drive business through the door. Text message advertising is easy to implement and drives measurable results for your business. So get started today and change your business for the better.

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Source by John Bauersfeld

Fisher-Price P4326 Meine erste Toilette Töpfchen und Toilettensitz mit Musik und Soundeffekten Toilettentrainer für Kleinkinder

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FISHER PRICE babygear Erste Toilette. Jetzt klappt der Übergang von Töpfchen zur Toilette spielend leicht. Realistische Elemente sprechen jedes Kind an. Die Lerntoilette reagiert beim Hoch- und Herunterklappen des Toilettendeckels, beim Ziehen der Spülung oder beim Abrollen des ‚Toilettenpapiers‘ mit Sätzen, Musik und Soundeffekten. Mit drei Lernstufen: Anfangs als frei stehende Toilette, dannohne die Fußteile als Toilettensitz und schließlich nur mit Sitz und Deckel auf der Erwachsenentoiletten benutzbar. Die Schale wird zum Reinigen einfach aus dem Sitz herausgenommen. 3 Alkali-Batterien AA (399.007.0) sind erforderlich. Für Kleinkinder ab 9 Monate.Durch die kleine Toilette mit realistischen Elementen fühlen sich die Kleinen schon ganz groß
Mit lustigen Sätzen, Musik und Soundeffekten wird selbst der Toilettengang zum Vergnügen
Sitzhöhe ca 18 cm Auch auf einem normalen Toilettensitz benutzbar Einfach zu reinigen



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