Keywords
X-Ray Transients: Be Stars
X-Ray Transients: Accretion
X-Ray Transients: Accretion
How to Cite
On the hard, pulsating X-ray transients. (1990). Revista Mexicana De Astronomía Y Astrofísica, 21(1), 467. https://astronomia.unam.mx/journals/rmxaa/article/view/1990rmxaa..21..467j
Abstract
It is shown that the X-ray luminosities observed in Be/X-ray systems can be explained by accretion from the extended, equatorially-concentrated, expanding envelope of the Be companion.Similar Articles
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