X-ray variability coherence: How to compute it, what it means, and how it constrains models of GX 339-4 and cygnus X-1

Astrophysical Journal

Volumn 474, Issue 1 PART II, 1997, Pages

  Vaughan, Brian A ^a   Nowak, Michael A ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF COLORADO   (United States)

Author keywords

Black hole physics; Methods: statistical; X rays: stars

Indexed keywords

EID: 26344470735     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310430     Document Type: Article

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