Viscosity mechanisms in accretion disks

Science

Volumn 288, Issue 5473, 2000, Pages 2022-2024

  Menou, Kristen ^a  

^a PRINCETON UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; GAS ANALYSIS; MATHEMATICAL ANALYSIS; PRIORITY JOURNAL; TURBULENT FLOW; VISCOSITY;

EID: 0034674719     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.288.5473.2022     Document Type: Article

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24. cold in the quiescent disk of the low q dwarf nova WZ Sge, which is orders of magnitude less than what is usually inferred for other dwarf novae [J. Smak, Acta Astron. 43, 101 (1993)].
25. I thank S. Balbus, C. Gammie, J. Goodman, B. Hansen, and R. Narayan for useful discussions. Supported by NASA through Chandra postdoctoral fellowship grant PF9-10006 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-39073.