CygX-1/A candidate of the black hole |
| |
Authors: | Minoru Oda |
| |
Institution: | (1) Institute of Space and Aeronautical Science, University of Tokyo, Komaba, Meguro-ku, 153 Tokyo, Japan |
| |
Abstract: | Among discrete galactic X-ray sources, Cyg X-1 has been noted for its peculiar features in several respects. It is one of
the few sources with a hard power law spectrum extending beyond several hundred keV. Cyg X-1 also distinguishes itself by
its profound time variability over a wide range of time scales. The most remarkable incident was that its optical identification
with a spectroscopic binary HDE226868 has led to a presumption that it is a black hole. This possibility has induced continuous
interests in the physical character of this source in conjunction with the nature of the black hole. The purpose of this paper
is to summarize presently available pieces of knowledge on this source to help the design of future experimental and theoretical
works, while the complexity of the source characteristics still has prevented us to construct a clear, coherent picture of
this source in spite of the fact that numerous observational facts have been accumulated. |
| |
Keywords: | |
本文献已被 SpringerLink 等数据库收录! |
|