Microquasars pp 169-174 | Cite as

Disk-Corona Interactions in Soft Spectral States of Black Hole Binaries

  • Piotr T. Życki
Conference paper

Abstract

Re-analysis of some archival X-ray data of black hole binaries in soft spectral states is presented. Results of detailed spectral fitting, including proper physical description of the X-ray reprocessed component, indicate that in most cases the soft, thermal disk emission cannot be described by a simple multi-color blackbody model. Additional Comptonization of those seed photons provides an acceptable description of the soft component, implying a presence of a warm (kT e ∼ 1 keV), mildly optically thick (τ ∼ 10) phase of accreting plasma.

Combined spectral/temporal analysis of GRS 1124-68 during ‘flip-flop’ transitions in very high state suggests that the optically thick accretion flow can proceed in (at least) two modes giving the same time-integrated behaviour (i.e. energy spectra) but very different timing behaviour.

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References

  1. Ebisawa, K., et al.: 1994, Puhl. Astron. Soc. Jpn. 46, 375.ADSGoogle Scholar
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  3. Takizawa, M., et al.: 1997; Astrophys. J. 489, 272.ADSCrossRefGoogle Scholar
  4. Zycki, P.T., Done, C. and Smith, D.A.: 1998, Astrophys. J. 496, L25.ADSCrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media New York 2001

Authors and Affiliations

  • Piotr T. Życki
    • 1
  1. 1.N. Copernicus Astronomical CenterWarsawPoland

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