Stellar disruption by a supermassive black hole: Is the light curve really proportional to t-5/3?

Monthly Notices of the Royal Astronomical Society

Volumn 392, Issue 1, 2009, Pages 332-340

  Lodato, G ^a   King, A R ^a   Pringle, J E ^a,b  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

Black hole physics; Galaxies: nuclei; Hydrodynamics

Indexed keywords

ANALYTICAL MODELS; BLACK HOLES; GALAXIES; GRAVITATION; LUMINANCE;

BLACK HOLE PHYSICS; DENSITY STRUCTURES; GALAXIES:NUCLEI; LIGHT CURVES; SOLAR TYPE STARS; STARS: BE; STELLAR MODELING; STELLARS; SUPERMASSIVE BLACK HOLES; TIME EVOLUTIONS;

STARS;

EID: 57849116440     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14049.x     Document Type: Article

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