The new model of a tidally disrupted star: Further development and relativistic calculations

Monthly Notices of the Royal Astronomical Society

Volumn 338, Issue 1, 2003, Pages 147-155

  Ivanov, P B ^a,d   Chernyakova, M A ^b,d,e   Novikov, I D ^c,d,f,g  

^a QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^b UNIVERSITY OF GENEVA   (Switzerland)

^c THEORETICAL ASTROPHYSICS CENTER   (Denmark)

^d LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^e UNIVERSITÉ DE GENÈVE   (Switzerland)

^f University Observatory ^*  (Denmark)

^g NORDITA   (Denmark)

Author keywords

Black hole physics; Galaxies: Nuclei

Indexed keywords

BLACK HOLES; EQUATIONS OF STATE; GALAXIES; GRAVITATION; LAGRANGE MULTIPLIERS; RELATIVITY;

BLACK HOLE PHYSICS; DYNAMICAL EQUATION; FURTHER DEVELOPMENT; GALAXIES:NUCLEI; LAGRANGIAN MODELS; ONE-DIMENSIONAL; RELATIVISTIC CALCULATIONS; SELF-CONSISTENT DERIVATION; SEMI-ANALYTICAL MODEL; THREE-DIMENSIONAL (3D) MODEL;

STARS;

EID: 0141923476     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06028.x     Document Type: Article

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