Spectroscopic Monitoring of the Be/X‐Ray Pulsar X Persei/4U 0352+309 with theOrbiting and Retrievable Far and Extreme Ultraviolet Spectrometer SPASII and theIUE

Author:

Smith Myron A.,Roche Paul

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. An application of the Ghosh & Lamb model to the accretion-powered X-ray pulsar X Persei;Publications of the Astronomical Society of Japan;2018-09-06

2. The Orbit of X Persei and Its Neutron Star Companion;The Astrophysical Journal;2001-01

3. Astrophysics in 1999;Publications of the Astronomical Society of the Pacific;2000-04

4. The Spectral Distribution of Be/X-ray Transients Implies Supernova Kicks;International Astronomical Union Colloquium;2000

5. Long-term Variability in Be-Star disks;International Astronomical Union Colloquium;2000

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