Why Laser Hair Removal Is Worth Preferring Over Other Techniques

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Growth of hair on face, chest, legs and arms can be daunting for people due to many reasons. Not only women, but men too wish to get rid of these undesired hairs to have an expressive and beautiful skin. Laser hair removal is a relatively newer process of removing hair from different body parts. A skilled specialist can help one obtain following benefits of removing hair with laser application.

Higher Efficacy
Hair removal through laser treatment has been accepted as a more effective technique than electrolysis, waxing and many such techniques. One can get better results with laser treatment to obtain skin that can be showcased to achieve acclaim and some flattering compliments.

Work for Different Body Parts
Laser hairs removal works for removal of hair from different body parts. While facial removal is quite popular with laser treatment, one can get it performed for sensitive body parts, including breasts, armpits and so on.

Less Hair Removal Pain
A serious drawback of conventional processes has been the pain associated with them. Laser Hair Removal is one technique which doesn't cause pain even while removing hair from the most sensitive body parts. This is one of the top reasons for people to get attracted towards this technique.

Suitable for All
Laser Hairs Removal for Women is popular and at the same time, laser hair removal for men is also gaining popularity for the ease and great results associated with the treatment. Men, not only from the world of glamor but the common men too are interested in removing hair from their chests, backs, legs and other body parts these days. Laser treatment is a wonderful solution for both the genders.

Fast Procedure per Session
Though, laser removal may require one to undergo 3 to 4 sessions, but time required per session is short. Moreover, one doesn't need to relax after getting treated using laser and can move to any place immediately after the session is over. As a result, it is a time-effective approach for people leading a busy life.

Permanent Results
With the advancement of technology, it is possible to obtain permanent results with laser removal. Even if the hairs re-grow after some time, the texture of new hairs is soft and can be easily removed once again.

In order to remove all these benefits of laser hair removal, you must obtain it from an authorized laser treatment clinic with specialized teams. Make sure you learn about things like number of sessions required and suitability of the treatment for your skin type before undergoing the treatment.

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Ocean Digital DB332 DAB/DAB + / FM-Radio mit Lautsprecher, AUX-IN, Audio Out, Kopfhöreranschluss, bis zu 40 voreingestellten Sendern, Holzgehäuse (Nussbaum)

Ocean Digital DB332 DAB/DAB + / FM-Radio mit Lautsprecher, AUX-IN, Audio Out, Kopfhöreranschluss, bis zu 40 voreingestellten Sendern, Holzgehäuse (Nussbaum)

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DB332 ist ein brillantes Holz-DAB-Radio! Eingebaut mit DAB + / DAB und FM.
Das Radio ermöglicht die Speicherung von bis zu 20 DAB- und 20 UKW-Sendern. Passen Sie die Liste der Voreinstellungen an Ihre Hörgewohnheiten an und widmen Sie den 4 Voreinstellungstasten Ihren Favoriten.

Die moderate Größe des Radios passt problemlos in die Küche, das Wohnzimmer oder das Schlafzimmer.
Der Ton ist gut für seine Größe, klar und laut. Möchten Sie zuhören, ohne andere zu unterbrechen? Schließen Sie Ihren Kopfhörer an die 3,5-mm-Kopfhörerbuchse des Radios an. Es besteht auch die Möglichkeit, Ihre vorhandene Stereoanlage über den 3,5-mm-Audioausgang anzuschließen. Darüber hinaus bietet die Teleskopantenne einen besseren und stabileren Empfang.

Der DB-332 ist gut verarbeitet und wurde mit größter Sorgfalt für Radiohörer entwickelt, um die Verwendung des Radios mit Funktionen zu vereinfachen, die praktisch genug sind. Holen Sie sich noch heute einen, um die Zufriedenheit beim Zuhören zu genießen!

Eigenschaften:
– DAB / DAB + / Digitales UKW-Radio mit Teleskopantenne
– 20 Voreinstellungen für DAB und 20 Voreinstellungen für UKW
– 3,5-mm-AUX-Eingang, Audioausgang, Kopfhörer
– Eingebauter Lautsprecher
– Zwei Farben erhältlich: Schwarz + Weiß / Walnuss + Weiß
– Sleep Timer
– Uhrzeit- / Datumsanzeige während der Wiedergabe und im Standby-Modus
– Dimmbares Display
– Vier Sprachoptionen: Englisch, Französisch, Deutsch, Italienisch

Technische Spezifikation:
Modell: DB-332
Leistungsaufnahme: 5V 1A
DAB-Frequenzbereich: 174.928MHz (5A) – 239.200MHz (13F), unterstützt DAB und DAB +
UKW-Frequenzbereich: 87,5-108 MHz
Audioausgangsleistung: 1 X 3 W RMS
Audioausgang: 3,5-mm-Kopfhöreranschluss, 3,5-mm-Audioausgang
Geräteabmessung: 187 x 109 x 116 mm (L x H x T)

Was ist in der Verpackung enthalten?
1 X DB-332 DAB-Radio
1 X Netzteil
1 X Benutzerhandbuch
Unterstützt DAB, DAB + und Digital FM Radio
4 dedizierte voreingestellte Tasten für den schnellen Zugriff auf Ihre beliebtesten Kanäle.Ermöglicht das Speichern von bis zu 40 voreingestellten Sendern, 20 auf DAB und 20 auf UKW
2 Drehknöpfe – Separater Lautstärkeregler und Abstimm- / Auswahlknopf. Zeit- und Datumsanzeige beim Abspielen des Radios
3,5-mm-AUX-Eingang und -Audioausgang – Hören Sie Ihre eigene Musik, indem Sie Ihr Telefon / Tablet / MP3-Player über den AUX-Eingang anschließen, oder schließen Sie externe Aktivlautsprecher über den Audioausgang an
Weitere Funktionen – Klares Negativ-Display und dimmbare Hintergrundbeleuchtung, Standby-Uhr, Vier Sprachen verfügbar, Sleep-Timer-Einstellung, 3,5-mm-Kopfhöreranschluss, Premium-Holz



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Shark Cove's Scuba Diving Beach on Oahu

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Named by the Scuba Diving Magazine as one of the "Top Twelve Shore Dives in the World," Shark's Cove at Kalalua Point in North Coast Oahu is definitely one of the island's best shore dives. The name might scare you off, but Shark's Cove is far from being homed by sharks. Instead, the name was derived from the way the cove's lava rock formation appears as seen from the air: it either looks like the head of a shark, or the remains of what a shark has bitten off.

The left side of the cove is where you enter. The rock and coral formations to the entry point are sharp; visitors are advised to wear shoes or reef walkers. However, entering the dive is fairly easy and leads you right out the lava tubes. Underwater, get ready to be amazed by the maze-like cave and cave and lava tube network, ledges, and smooth boulders. One of the best features of Shark's Cove is its clear blue water and visibility that ranges from 50-100 feet — just perfect enough for viewing the reef's rich marine sea life. The reef features more species of fish and more varied marine life than most dive shores in the island. Butterfly fishes, leviathan, needle fish, eels, perch, eagle rays, fluorescent crabs, trigger fish, and sea turtles are some of the sea creatures to delight any diver here.

Shark Cove's only downside is that it can only be dived in summer when ocean water is calm. Because it is located between the big wave surfing spots of Banzai Pipeline and Waimea Bay, diving conditions in Shark's Cove become dangerous during winter months when North Shore waves can rise to more than 20 feet high. Big breaking waves also reduce the reef's visibility. Even in summer, the coves sometimes get choppy. At any time of the year, when you see large ocean waves, it is strongly advised that you stay away from the rocks. And if you walk away from the rocks, walk away facing the sea. The waves are unpredictable, and can get dangerously big at any moment.

Dives in the cove are free. But because of Shark's Cove popularity, parking lots tend to fill up quickly. Still, Shark's Cove is not as crowded as the nearby Hanauma Bay.

If diving is not your cup of tea, there are tide pools nearby; they are excellent for swimming. The seascape is also stunning. You can spend your time just watching the ocean activity and the cove's rock formations, and already be blown away.

Services and amenities: free parking, rest rooms and showers, no lifeguards, small food and drink shops.

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Source by Kani Amea

adidas Herren Coast Star Sneaker, Weiß Core Black/Footwear White 0, 47 1/3 EU

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ADIDAS COAST STAR [WHITE BLACK WHITE]Der adidas Coast Star ist ein cleaner Sneaker aus weichem Leder. Er ist niedrig geschnitten und besitzt die typischen gezackten 3-Streifen an der Seite. Schnürung und Ferse wurden verstärkt und sorgen so für eine gute Haltbarkeit. Die adidas Logos an Zunge und Ferse runden das schlichte Design ab. Obermaterial Leder, Synthetik Innenfutter Textil, Synthetik Sohle Synthetik verstärkte Ferse und Schnürung adidas-Label an Zunge und Ferse dämpfende Einlegesohle EE8908Hochwertiges Glattleder ist strapazierfähig und langlebig
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Der Coast Star für Herren von Adidas ist ein angesagter Sneaker im minimalistischen Design und der Hingucker in deinem Streetwear-Outfit.



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Unwanted Pop-Ups: Disguising an Erect Penis

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For some men, there’s never a „wrong“ time to have an erect penis. An exhibitionist may always welcome a very visible „pup tent,“ or a man who is totally at ease may view penis pop-ups in social or professional situations as just a fact of life. But many men do find that there are times and places where an erect penis is an unwanted distraction. While not a penis health issue per se, an unwanted erect penis can be a problem for some men, so knowing how to handle this situation can make them feel more comfortable with their penis in general.

An adolescent experience

Many times, an adult’s discomfort with an unwanted erect penis goes back to their adolescence. Countless teen-age boys have stood in front of classrooms with pop-ups tenting their flies. They have been forced to make a report or awkwardly work out math problems while awkwardly keeping their boner from touching the chalkboard or smart board. And while doing so, they have endured snickers from their classmates and later may have to put up with nicknames from other boys.

Therefore, when an erect penis pops up in their adult lives – as they are giving a presentation at work or meeting their girl friend’s father for the first time – their previous experience greatly increases their embarrassment and discomfort.

Tips

So what can a guy do to help lessen the awkwardness he experiences in such situations? The following tips may prove helpful.

Go baggy. Sure, when wanting to impress a partner or potential partner, tight pants can be the way to go. But if a guy is worried about pop-ups, he wants to be able to disguise or hide that erect penis. Baggy trousers allow for the penis to expand and stand at attention without attracting undue notice. Sure, some guys are so heavily endowed that this doesn’t work, but for guys of average size, it can make all the difference.

Choose underwear carefully. Every man is different, and his penis has its own way of reacting to different stimuli. For some guys, the way the penis rub against boxers may be more arousing than with briefs – so choosing briefs may be an option. Cotton may cause a different reaction than synthetics. And if a dude associates a certain pair of underwear with hot sex – leave it at home on days when an erection is not on the menu.

Masturbate. If a man is really worried, he may want to simply masturbate a half hour or so before that big presentation or before that important cocktail party. Masturbating will decrease the chance that a penis will get all aroused and restless for the next couple of hours.

Meditate. Some guys find that meditating or practicing yoga can also help them to better control pop-ups. Learning what breathing exercises or visualizations can have a desired temporary „dampening“ effect can be invaluable.

Look for hiding places. Scout the room for opportunities to disguise a persistent bulge in the crotch. If making a speech, take advantage of a podium to hide behind it if the penis gets playful. Standing behind a high-backed chair at a party can do wonders, as can sitting and crossing one’s legs. As a last resort, standing with one’s hands clasped in front of the crotch may draw attention to the area – but those with big enough hands may be able to disguise the fact that there’s an active penis behind them.

An erect penis at the right time is wonderful, so a guy shouldn’t let unwanted pop-ups put him off his game. He still wants to regularly use a superior penis health creme (health professionals recommend Man 1 Man Oil, which is clinically proven mild and safe for skin) to encourage greater penis health. The best cremes will contain L-carnitine, an amino acid which has neuroprotective abilities to help maintain a proper degree of penis sensitivity. The crème should also include, vitamin C, a key component of collagen, a tissue in the body that gives skin its tone and elasticity.

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Funko 34390 Pop-Vinyl: South Park W2: Mr Hankey, Mehrfarbig

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Mr. Hankey Vinyl Figure 21 South Park Funko Pop! für Unisex in Standard aus Vinyl. Offiziell lizenziertes Produkt.POP! Vinyl.
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So Exactly What Is The Difference Between 10 Meter Radio And CB Radio?

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Over the past few years the line between traditional CB radio and 10 meter radio has become blurred. Phrases like ’10 meter CB radio‘ and ‚export radio‘ have irrevocably woven themselves into the vocabulary. Despite widespread use of both technologies many users have no idea what the real differences are.

A traditional CB operates on the 11 meter band at about 27mhz. This gives it 40 channels ranging from 26.965mhz on channel 1 to 27.405mhz on channel 40. The distinctive characteristic of CB is that access to these frequencies is unrestricted by the FCC and available to anyone. Thus the term ‚Citizens Band‘.

However although access is unrestricted, use of these frequencies is another matter. Users are required to adhere to certain codes of conduct and severe hardware limitations. By FCC rule no CB transmitter may exceed 4 watts of transmitting power. A smart operator may use a high quality antenna to ‚get out‘ further but increasing output by almost any other means is prohibited.

By contrast 10 meter radio access is restricted but the allowable hardware is not as limited. 10 meter radios operate on frequencies ranging from 28mhz to 29.7mhz. To access 10 meter radio frequencies you are required to obtain an amateur or ‚ham‘ radio license from the FCC. Such licenses are relatively easy to get and usually free of charge. Certain 10 meter radios also operate on FM radio frequencies which will require an even more advanced license. The hardware involved in 10 meter radio can be quite impressive. Unlike CB communications the FCC considers the 10 meter band acceptable for long range communication, many radios offer over 100 times the transmitting power of a traditional CB transmitter.

So why has the line between the two become blurred? Many CB operators dislike the severe restrictions placed on CB transmission output. Manufacturers responding to this desire have produced 10 meter radios that look and operate exactly like a standard CB. These new radios are easily modified to operate on CB radio frequencies which is probably what both the manufacturer and operator both had in mind when it was purchased. It is important to note that such modifications are against FCC rules.

The term ‚export radio‘ is used to refer to these new CB radio style 10 meter radios. The catch is that these radios are supposed to be marketed for export use only. Many other countries do not have such severe restrictions on transmitting power as does the United States.

Although there is a large amount of public desire to allow greater transmitting power amongst CB radio users the FCC is very unlikely to change its policy anytime soon. The FCC regards CB radio as a short range communication device and does not want high powered transmissions interrupting local communications between other operators. This viewpoint will almost certainly preclude any change in policy any time in the near future. By knowing the difference between 10 meter and CB radio, and how you intend to use your new equipment, determining which is the right model for you should be clear.

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Source by Jeff C Thorson

Hubble Uncovers An Elusive, Doomed Star

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Stars are like people–they send their dazzling light through the Cosmos for a little while, but do not last forever in the universal tragicomedy of our existence. Supernovae herald the fatal explosions of massive stars that have come to the end of that long stellar road, after having burned their necessary supply of nuclear-fusing fuel–and have perished brilliantly and beautifully, as they scream explosively into oblivion. One of the ways that astronomers search for clues, hinting at how these massive stars blow themselves up, is to go on the hunt for what is termed the progenitor star of the supernova. In order to accomplish their quest, astronomers carefully sift through archival telescope images and try to determine the precise location and identity of the progenitor star before it blew itself to pieces. In November 2018, for the first time, a California Institute of Technology (Caltech) team of astronomers in Pasadena announced that they have likely discovered just such a stellar progenitor for a supernova class known as Type Ic (pronounced „one-C“). Of all the classes of supernovae, this is the only one that did not have a known stellar progenitor until their discovery. For this reason, its identification was considered by astronomers to be a kind of Holy Grail.

The Type Ic supernova, dubbed SN 2017, was first spotted in May 2017 by astronomers using the Tenagra Observatories in Arizona. It is situated in a spiral galaxy named NGC 3938, that is located about 65 million light-years from Earth. The Caltech astronomers were able to successfully track this supernova’s progenitor using archival images from NASA’s Hubble Space Telescope (HST), obtained back in 2007.

„An alert was sent out when the supernova was initially found. You can’t sleep once that happens and have to mobilize to try to find the progenitor to the explosion. Within a few weeks after the supernova was discovered, we found a candidate using both new and archival Hubble images. The new images were essential for pinpointing the candidate progenitor’s location,“ noted Dr. Schuyler Van Dyk in a November 15, 2018 JPL Press Release. Dr. Van Dyk is a staff scientist at IPAC, which is a science and data center located at Caltech.

The progenitor turned out to be a luminous and very hot star, and it is thought to be either a singly massive star 48 to 49 times solar-mass or a massive binary system in which the star that went supernova weighed-in at a hefty 60 to 80 times the mass of our Sun.

Type Ic Supernovae

Type Ic supernovae, and their close cousins Type Ib supernovae, are classifications of supernovae that result from the explosive core collapse of massive stars. These doomed stars have flung off, or have been more gently stripped of, their outer envelope of hydrogen gas. When Type Ic and Type Ib supernovae are compared to Type Ia supernovae, they do not show the absorption line of silicon. When compared to Type Ib, Type Ic supernovae are believed to have lost more of their original gaseous envelope, including most of their helium. Astronomers usually refer to the two types as „stripped core-collapse supernovae.“

All stars, regardless of their mass, churn out energy by way of the process of the nuclear-fusion of atomic elements, which creates heavier elements out of lighter ones. Unlike our relatively small Sun, more massive stars contain suffient mass to fuse elements that have an atomic mass greater than hydrogen and helium–albeit at progressively greater and greater temperatures and pressures. This increase results in a shorter „life“ for massive stars. Small stars, like our Sun, „live“ on the hydrogen-burning branch of the Hertzsprung-Russell Diagram of Stellar Evolution for about 10 billion years. In dramatic contrast, massive stars „live“ fast and „die“ young. The more massive the star, the shorter its „life“. A hefty star fuses increasingly heavier atomic elements, commencing with hydrogen and helium, and then progressing through the familiar Periodic Table until a core of iron and nickel is formed. Because nuclear-fusion of iron or nickel manufactures no net energy output, no additional fusion can occur, leaving the nickel-iron core of the doomed massive star inert. Due to the lack of energy output creating the necessary outward thermal pressure to keep the heavy star bouncy against the relentless inward pull of its own gravity, the core shrivels. When the compacted mass of the inert iron and nickel core exceeds what is called the Chandrasekhar Limit of 1.4 solar-masses, radiation pressure cannot counter gravitational compression, and a cataclysmic implosion of the core occurs within seconds. At this point, lacking the support of the now-imploded inner core, the outer core of the erstwhile massive star collapses inward under the merciless force of gravity and attains a velocity of up to 23% the speed of light. The sudden, dramatic compression increases the temperature of the inner core to as much as 100 billion Kelvins. The collapse of the inner core is stopped by neutron degeneracy, resulting in the implosion to rebound and bounce outward. The energy of the expanding shock wave disrupts the overlying stellar material and accelerates it to escape velocity. A horrific, brilliant Type II supernova occurs, and where once there was a massive star there is a star no more. Depending on the hefty progenitor star’s mass, the souvenir that it leaves behind to remind the Universe of its former existence will be either a dense, city-sized neutron star or a stellar mass black hole.

Small stars go to their inevitable grand finale differently. Type Ia supernovae, unlike core-collapse Type II supernovae, do not originate from the funeral pyre of a massive progenitor star. Type Ia supernovae are the catastrophic leftovers of small stars, like our Sun, that have perished to become a type of dense stellar relic termed a white dwarf. Our Sun will never perish in the terrible beauty born from a Type Ia blast. This is because our Sun is a solitary Star. However, when small stars of our Sun’s mass dwell in a binary system with another still-living star, it’s a party ready to happen. If the dense, vampire-like white dwarf relentlessly gravitationally sips up its companion star’s material, it pays for its crime by „going critical.“ That is, the murderous white dwarf steals enough mass from its companion to attain the critical mass to blow itself to pieces–just like its more massive stellar kin. Alternatively, a Type Ia supernova can also occur when a duo of white dwarfs, composing a binary system, blast into one another. When this happens, it also results in a horrific Type Ia supernova explosion.

Piecing together how each of these supernova types (Type II, Type Ib, Type Ia, and Type Ic) occur provides a greatly improved understanding of how the most massive stars in the Universe evolve.

Uncovering An Elusive, Doomed Stellar Progenitor

Type Ic supernovae occur with the most massive stars. But we were surprised by how massive this one appears to be, and especially by the possibility of a massive double-star system as the progenitor. Although theories have existed for the last three decades that Type Ic supernovae could be the explosions of very massive single stars, alternative, more recent theories point toward stars of lower mass in binary systems as being the origins of these explosions,“ Dr. Van Dyk explained in the November 15, 2018 Caltech Press Release.

Type Ib and Type Ic differ from Type II because their stellar progenitors lose their outer envelopes of material surrounding their central cores before going supernova. Type Ib and Ic also differ from each other slightly in chemical composition.

„The origins of such explosions are relevant to the entire astronomical community, not just supernova researchers. The results have implications on ideas from star formation to stellar evolution and feedback into the galaxy,“ Dr. Ori Fox commented in the November 15, 2018 Caltech Press Release. Dr. Fox is a Support Scientist at the Space Telescope Science Institute (STScI) in Baltimore, Maryland.

Dr. van Dyk continued to note in the same Press Release that „Astronomers have been trying to find this progenitor for some 20 years. Humans wouldn’t be here without supernovae–they make the chemical elements from which we are made.“

The astronomers also commented that they should be able to confirm with certainty whether they have identified the correct progenitor to the Type Ic explosion within a few years, using Hubble or the upcoming James Webb Space Telescope, planned to launch in 2021. As the supernova dims as predicted, the astronomers will have a clearer view of the region surrounding it. If the luminous progenitor candidate was correctly identified in archival images, then it will have disappeared and should not be detected in the new images. If the scientists still see the candidate progenitor, that means it was misidentified and some other hidden star was the true culprit behind the cataclysmic blast.

In Memory of Mark.

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Fire 7-Tablet mit Alexa, 17,7 cm (7 Zoll) Display, 8 GB (Schwarz), mit Spezialangeboten

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