X-Ray Pulsar的封面
书籍主题:

X-Ray Pulsar

Betascript Publishing (2010-11-07 )

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ISBN-13:

978-613-0-57447-5

ISBN-10:
6130574479
EAN:
9786130574475
书籍语言:
英文
作品简介:
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. X-ray pulsars or accretion-powered pulsars are a class of astronomical objects that are X-ray sources displaying strict periodic variations in X-ray intensity. The X-ray periods range from as little as a fraction of a second to as much as several minutes. An X-ray pulsar consists of a magnetized neutron star in orbit with a normal stellar companion and are a type of binary star system. The magnetic field strength at the surface of the neutron star is typically about 1012 gauss, over a trillion times stronger than the strength of the magnetic field measured at the surface of the Earth (0.6 gauss). Gas is accreted from the stellar companion and is channeled by the neutron star's magnetic field on to the magnetic poles producing two or more localized X-ray hot spots similar to the two auroral zones on the Earth but far hotter.
出版社 :
Betascript Publishing
网址:
https://www.betascript-publishing.com/
出版发行由:
Lambert M. Surhone, Mariam T. Tennoe, Susan F. Henssonow
页码 :
112
发表日期:
2010-11-07
现货:
备有现货
类别:
物理 ,天文学
价格:
39.00 €
关键词:
Astronomy, X-ray, Magnetic Field, Aurora (Astronomy), Stellar Wind

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