Spotty neutron stars.Spinning up to hundreds of times a second and packing an entire sun's mass into a sphere just slightly wider than the length of Manhattan, a neutron star neutron star, extremely small, extremely dense star, about double the sun's mass but only a few kilometers in radius, in the final stage of stellar evolution. Astronomers Baade and Zwicky predicted the existence of neutron stars in 1933. ranks among the weirdest objects in the universe. Astronomers have for the first time discerned a hot spot on the surfaces of three of these cosmic oddities. The X-ray--emitting spots, estimated to range in size from the area of a football field to that of a golf course, are the smallest features that astronomers have detected on objects so far away, in this ease from 500 to 2,000 light-years from Earth. Researchers have proposed that such a hot spot arises when the strong magnetic fields magnetic fields, n.pl the spaces in which magnetic forces are detectable; created by magnetostrictive ultrasonic scalers to cause the tips of instruments such as ultrasonic scalers to vibrate. around a cooling neutron star funnels energy back onto a small patch of the star's surface. According to according to prep. 1. As stated or indicated by; on the authority of: according to historians. 2. In keeping with: according to instructions. 3. this theory, this magnetic funneling happens in the same way on all neutron stars and all hot spots hot spots acute moist dermatitis. should be about the same size. Patrizia Caraveo of the National Institute of Astrophysics astrophysics, application of the theories and methods of physics to the study of stellar structure, stellar evolution, the origin of the solar system, and related problems of cosmology. in Milan, Italy, and her colleagues detected the rapid rise and fall of X rays from hot spots on three neutron stars--Geminga, PSR PSR Pulsar PSR Poster PSR Physicians for Social Responsibility PSR Psychosocial Rehabilitation PSR Pacific School of Religion PSR Policy and Survey Research PSR Project Study Report PSR Pre-Sentence Report PSR Pressure-State-Response PSR Puget Sound Region B0656+14, and PSR B1055-52--using the superlative X-ray-collecting mirror of the orbiting XMM-Newton Observatory. The team calculates that the hot spots on the neutron stars vary from 100 meters to as much as 4 kilometers across. "It's impressive that we can see such small spots from so far away with this kind of detail," says Dong Lai of Cornell University. However, he says, the apparent size difference in the hot spots might result from the simplifying assumptions by Caraveo's team. More-nuanced models and more data ought to determine whether the spots are the same size, he says. Caraveo's team reports the findings in the April 20 Astrophysical Journal.--R.C. |
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