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DOI10.1126/science.275.5296.49
Generation of x-rays from comet C/Hyakutake 1996 B2
Bingham R.; Dawson J.M.; Shapiro V.D.; Mendis D.A.; Kellett B.J.
发表日期1997
ISSN0036-8075
起始页码49
结束页码50
卷号275期号:5296
英文摘要The instability resulting from the relative motion of newly picked-up cometary photoions and the solar wind generates lower hybrid waves that are capable of accelerating electrons to the keV range of energies. These electrons may be responsible for the x-rays from comet C/Hyakutake 1996 B2 seen by the Rontgen X-ray Satellite. The inferred x-ray photon power depends on the electron energy, with keV electrons providing values of photon power two orders of magnitude greater than 100 eV electrons. These observations and in particular, spectral resolution of the x-rays, should provide more insight into the composition of the comet.
英文关键词article; astronomy; electron; energy; photon; priority journal; X ray
语种英语
来源期刊Science
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/243048
作者单位Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX, United Kingdom; Department of Physics, University of California, Los Angeles, CA 90024, United States; Department of Physics, Univ. of California at San Diego, San Diego, CA 92092, United States; Dept. of Elec. and Computing Science, Univ. of California at San Diego, San Diego, CA 92092, United States
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Bingham R.,Dawson J.M.,Shapiro V.D.,et al. Generation of x-rays from comet C/Hyakutake 1996 B2[J],1997,275(5296).
APA Bingham R.,Dawson J.M.,Shapiro V.D.,Mendis D.A.,&Kellett B.J..(1997).Generation of x-rays from comet C/Hyakutake 1996 B2.Science,275(5296).
MLA Bingham R.,et al."Generation of x-rays from comet C/Hyakutake 1996 B2".Science 275.5296(1997).
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