Ir directamente a la navegación principal Ir directamente a la búsqueda Ir directamente al contenido principal

Accretion of stellar winds in the galactic centre

  • J. Cuadra
  • , S. Nayakshin
  • , V. Springel
  • , T. Di Matteo

Producción científica: Capítulo del libro/informe/acta de congresoContribución a la conferenciarevisión exhaustiva

Resumen

We report a 3-dimensional numerical study of the accretion of stellar winds onto Sgr A*, the super-massive black hole at the centre of our Galaxy. Compared with previous investigations, we allow the stars to be on realistic orbits, include the recently discovered slow wind sources, and allow for optically thin radiative cooling. We find that the slow winds shock and rapidly cool, forming cold gas clumps and filaments that coexist with the hot X-ray emitting gas. The accretion rate in this case consists of two components: the hot quasi steady-state one, and the cold one that is highly variable on time-scales of tens to hundreds of years. Such variability can in principle lead to a strongly non-linear response through accretion flow physics not resolved here, making Sgr A* an important energy source for the Galactic centre.

Idioma originalInglés
Título de la publicación alojadaRelativistic Astrophysics Legacy and Cosmology - Einstein's
Subtítulo de la publicación alojadaProceedings of the MPE/USM/MPA/ESO Joint Astronomy Conference Held in Munich, Germany, 7-11 November 2005
EditoresBernd Aschenbach, Vadim Burwitz, Gunther Hasinger, Bruno Leibundgut
Páginas115-119
Número de páginas5
DOI
EstadoPublicada - 2008
Publicado de forma externa

Serie de la publicación

NombreESO Astrophysics Symposia
Volumen2008
ISSN (versión impresa)1431-2433
ISSN (versión digital)1611-6143

Huella

Profundice en los temas de investigación de 'Accretion of stellar winds in the galactic centre'. En conjunto forman una huella única.

Citar esto