On Be/X-ray binaries with an intermediate-mass black hole

Details On Be/X-ray binaries with an intermediate-mass black hole On Be/X-ray binaries with an intermediate-mass black hole

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010raa....10..672l&link_type=abstract

Research in Astronomy and Astrophysics, Volume 10, Issue 7, pp. 672-680 (2010).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We adopt the tidal truncation model proposed by Negueruela and Okazaki for Be/X-ray binaries to investigate the influence of intermediate-mass black holes (IMBHs) on Be-star disks. We show that the viscous decretion disks around Be stars are generally truncated ineffectively under the tidal force of IMBHs. Combining this with observations of Be/X-ray binaries, we suggest that Be/IMBH X-ray binaries may appear as recurrent luminous X-ray transients with quasi-periodic X-ray outbursts.

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