SciELO - Scientific Electronic Library Online

 
vol.43 número1The Kinematics of ARP 295 in Hα Emission: An Interacting Galaxy with Highly Asymmetric RotationLong gamma-ray burst prompt emission properties as a cosmological tool índice de autoresíndice de assuntospesquisa de artigos
Home Pagelista alfabética de periódicos  

Serviços Personalizados

artigo

Indicadores

Links relacionados

  • Não possue artigos similaresSimilares em SciELO

Bookmark

  • |

Revista mexicana de astronomía y astrofísica

versão impressa ISSN 0185-1101

Resumo

HUERTA, E. A.  e  MENDOZA, S. A Simple Accretion Model of a Rotating Gas Sphere onto a Schwarzschild Black Hole. Rev. mex. astron. astrofis [online]. 2007, vol.43, n.1, pp. 191-202. ISSN 0185-1101.

We construct a simple accretion model of a rotating gas sphere onto a Schwarzschild black hole. We show how to build analytic solutions in terms of Jacobi elliptic functions. This construction represents a general relativistic generalisation of the Newtonian accretion model first proposed by Ulrich (1976). In exactly the same form as it occurs for the Newtonian case, the flow naturally predicts the existence of an equatorial rotating accretion disc about the hole. However, the radius of the disc increases monotonically without limit as the flow reaches its minimum allowed angular momentum for this particular model.

Palavras-chave : ACCRETION, ACCRETION DISKS; HYDRODYNAMICS; RELATIVITY.

        · resumo em Espanhol     · texto em Inglês     · pdf em Inglês