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Contact Coby Customer Service. Find Coby Customer Support, Phone Number, Email Address, Customer Care Returns Fax, 800 Number, Chat and Coby FAQ. Speak with Customer. The light curves of gamma-ray bursts are extremely diverse and complex. No two gamma-ray burst light curves are identical, with large variation observed in almost. MEASURING VOLTAGE Most of the readings you will take with a multimeter will be VOLTAGE readings. Before taking a reading, you should select the highest range and if. Credit: NOAA. A wavelength is the distance between two consecutive peaks of a wave. This distance is given in meters (m) or fractions thereof. Download now!! ![]() Gamma- ray burst - Wikipedia. Artist's illustration showing the life of a massive star as nuclear fusion converts lighter elements into heavier ones. When fusion no longer generates enough pressure to counteract gravity, the star rapidly collapses to form a black hole. This is the official Dr. Richard Boylan website©. It contains reports, articles, and other information on the Star Visitors, on their starcraft (UFOs), and on the. NASA.gov brings you the latest images, videos and news from America's space agency. Get the latest updates on NASA missions, watch NASA TV live, and learn about our. Theoretically, energy may be released during the collapse along the axis of rotation to form a gamma- ray burst. In gamma- ray astronomy, gamma- ray bursts (GRBs) are extremely energetic explosions that have been observed in distant galaxies. They are the brightest electromagnetic events known to occur in the universe. A subclass of GRBs (the . The cause of the precursor burst observed in some of these short events may be the development of a resonance between the crust and core of such stars as a result of the massive tidal forces experienced in the seconds leading up to their collision, causing the entire crust of the star to shatter. All observed GRBs have originated from outside the Milky Way galaxy, although a related class of phenomena, soft gamma repeater flares, are associated with magnetars within the Milky Way. It has been hypothesized that a gamma- ray burst in the Milky Way, pointing directly towards the Earth, could cause a mass extinction event. Following their discovery, hundreds of theoretical models were proposed to explain these bursts, such as collisions between comets and neutron stars. These discoveries, and subsequent studies of the galaxies and supernovae associated with the bursts, clarified the distance and luminosity of GRBs, definitively placing them in distant galaxies. History. Vela satellites, which were built to detect gamma radiation pulses emitted by nuclear weapons tested in space. The United States suspected that the Soviet Union might attempt to conduct secret nuclear tests after signing the Nuclear Test Ban Treaty in 1. On July 2, 1. 96. UTC, the Vela 4 and Vela 3 satellites detected a flash of gamma radiation unlike any known nuclear weapons signature. As additional Vela satellites were launched with better instruments, the Los Alamos team continued to find inexplicable gamma- ray bursts in their data. By analyzing the different arrival times of the bursts as detected by different satellites, the team was able to determine rough estimates for the sky positions of sixteen bursts. The discovery was declassified and published in 1. The distribution is isotropic, with no concentration towards the plane of the Milky Way, which runs horizontally through the center of the image. Most early theories of gamma- ray bursts posited nearby sources within the Milky Way Galaxy. From 1. 99. 1, the Compton Gamma Ray Observatory (CGRO) and its Burst and Transient Source Explorer (BATSE) instrument, an extremely sensitive gamma- ray detector, provided data that showed the distribution of GRBs is isotropic—not biased towards any particular direction in space. The absence of any such pattern in the case of GRBs provided strong evidence that gamma- ray bursts must come from beyond the Milky Way. Astronomers considered many distinct classes of objects, including white dwarfs, pulsars, supernovae, globular clusters, quasars, Seyfert galaxies, and BL Lac objects. This suggested an origin of either very faint stars or extremely distant galaxies. Early searches for this afterglow were unsuccessful, largely because it is difficult to observe a burst's position at longer wavelengths immediately after the initial burst. The breakthrough came in February 1. Beppo. SAX detected a gamma- ray burst (GRB 9. The William Herschel Telescope identified a fading optical counterpart 2. Well before then, another major breakthrough occurred with the next event registered by Beppo. SAX, GRB 9. 70. 50. This event was localized within four hours of its discovery, allowing research teams to begin making observations much sooner than any previous burst. The spectrum of the object revealed a redshift of z = 0. Earth. The following year, GRB 9. SN 1. 99. 8bw), coincident in location, indicating a clear connection between GRBs and the deaths of very massive stars. This burst provided the first strong clue about the nature of the systems that produce GRBs. However, the revolution in the study of gamma- ray bursts motivated the development of a number of additional instruments designed specifically to explore the nature of GRBs, especially in the earliest moments following the explosion. The first such mission, HETE- 2. One of the most successful space missions to date, Swift, was launched in 2. More recently, the Fermi mission was launched carrying the Gamma- Ray Burst Monitor, which detects bursts at a rate of several hundred per year, some of which are bright enough to be observed at extremely high energies with Fermi's Large Area Telescope. Meanwhile, on the ground, numerous optical telescopes have been built or modified to incorporate robotic control software that responds immediately to signals sent through the Gamma- ray Burst Coordinates Network. This allows the telescopes to rapidly repoint towards a GRB, often within seconds of receiving the signal and while the gamma- ray emission itself is still ongoing. Some bursts are preceded by a . Many classification schemes have been proposed, but these are often based solely on differences in the appearance of light curves and may not always reflect a true physical difference in the progenitors of the explosions. However, plots of the distribution of the observed duration. Additional classes beyond this two- tiered system have been proposed on both observational and theoretical grounds. These account for about 3. In addition, there has been no association with supernovae. Such mergers might also be expected to produce kilonovae. This further suggests a very compact object as the source. Because these events constitute the majority of the population and because they tend to have the brightest afterglows, they have been observed in much greater detail than their short counterparts. Almost every well- studied long gamma- ray burst has been linked to a galaxy with rapid star formation, and in many cases to a core- collapse supernova as well, unambiguously associating long GRBs with the deaths of massive stars. They have been proposed to form a separate class, caused by the collapse of a blue supergiant star. The most studied ultra- long events include GRB 1. A and GRB 1. 11. 20. A. Energy from the explosion is beamed into two narrow, oppositely directed jets. Gamma- ray bursts are very bright as observed from Earth despite their typically immense distances. An average long GRB has a bolometric flux comparable to a bright star of our galaxy despite a distance of billions of light years (compared to a few tens of light years for most visible stars). Most of this energy is released in gamma rays, although some GRBs have extremely luminous optical counterparts as well. GRB 0. 80. 31. 9B, for example, was accompanied by an optical counterpart that peaked at a visible magnitude of 5. This combination of brightness and distance implies an extremely energetic source. Assuming the gamma- ray explosion to be spherical, the energy output of GRB 0. B would be within a factor of two of the rest- mass energy of the Sun (the energy which would be released were the Sun to be converted entirely into radiation). Rather, gamma- ray bursts are thought to be highly focused explosions, with most of the explosion energy collimated into a narrow jet. When a gamma- ray burst is pointed towards Earth, the focusing of its energy along a relatively narrow beam causes the burst to appear much brighter than it would have been were its energy emitted spherically. When this effect is taken into account, typical gamma- ray bursts are observed to have a true energy release of about 1. J, or about 1/2. 00. Solar mass (M. This is comparable to the energy released in a bright type Ib/csupernova and within the range of theoretical models. Very bright supernovae have been observed to accompany several of the nearest GRBs. Wolf–Rayet stars are candidates for being progenitors of long- duration GRBs. Because of the immense distances of most gamma- ray burst sources from Earth, identification of the progenitors, the systems that produce these explosions, is challenging. The association of some long GRBs with supernovae and the fact that their host galaxies are rapidly star- forming offer very strong evidence that long gamma- ray bursts are associated with massive stars. The most widely accepted mechanism for the origin of long- duration GRBs is the collapsar model. Matter near the star's core rains down towards the center and swirls into a high- density accretion disk. The infall of this material into a black hole drives a pair of relativistic jets out along the rotational axis, which pummel through the stellar envelope and eventually break through the stellar surface and radiate as gamma rays. Some alternative models replace the black hole with a newly formed magnetar. Eta Carinae and WR 1. There is strong evidence that some short- duration gamma- ray bursts occur in systems with no star formation and no massive stars, such as elliptical galaxies and galaxy halos. According to this model, the two stars in a binary slowly spiral towards each other because gravitational radiation releases energy. The infall of matter into the new black hole produces an accretion disk and releases a burst of energy, analogous to the collapsar model. Numerous other models have also been proposed to explain short gamma- ray bursts, including the merger of a neutron star and a black hole, the accretion- induced collapse of a neutron star, or the evaporation of primordial black holes. This event had a gamma- ray duration of about 2 days, much longer than even ultra- long GRBs, and was detected in X- rays for many months. It occurred at the center of a small elliptical galaxy at redshift z = 0. Margin Call. Money Management . A key way to avoid losses is learning how to avoid a margin. What is a Margin Call - thebalance. Learn what creates a margin call and more importantly how to avoid one for a more peaceful Forex trading career. 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