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Prospects for experimental research on black holes in binary systemsCygnus X-1, the single widely accepted example of a black hole in a binary system, is characterized by unusual X-ray properties. The X-ray spectrum of Cygnus X-1 is not cut off above 20 keV, as in most strong X-ray sources. Recent scintillation counter measurements reveal a power law spectrum extending from 40 to 200 keV with a photon spectral index of approximately 2.2. However, it is not clear that these and other X-ray properties of the system are related to the black-hole nature of Cygnus X-1. It is suggested that without a direct test to show that the mass of the compact object in other systems similar to Cygnus X-1 (Circinus X-1 and GX339-4) exceeds the limit of the neutron star mass, a better understanding of the accretion disk phenomenon must be achieved to demonstrate how the properties peculiar to these systems are related to the black hole nature of the compact object. Current accretion disk models are examined, including the alpha-accretion disk and two-temperature accretion disk models.
Document ID
19800053501
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Long, K. S.
(Columbia University New York, N.Y., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Astrophysics
Accession Number
80A37671
Funding Number(s)
CONTRACT_GRANT: NAS5-24152
CONTRACT_GRANT: NGR-33-008-102
Distribution Limits
Public
Copyright
Other

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