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The Case for Massive, Evolving Winds in Black Hole X-ray Binaries

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 نشر من قبل Joseph Neilsen
 تاريخ النشر 2013
  مجال البحث فيزياء
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 تأليف Joseph Neilsen




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In the last decade, high-resolution X-ray spectroscopy has revolutionized our understanding of the role of accretion disk winds in black hole X-ray binaries. Here I present a brief review of the state of wind studies in black hole X-ray binaries, focusing on recent arguments that disk winds are not only extremely massive, but also highly variable. I show how new and archival observations at high timing and spectral resolution continue to highlight the intricate links between the inner accretion flow, relativistic jets, and accretion disk winds. Finally, I discuss methods to infer the driving mechanisms of observed disk winds and their implications for connections between mass accretion and ejection processes.



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