Accretion of stellar winds in the galactic centre

J. Cuadra; S. Nayakshin; V. Springel; T. Di Matteo

Accretion of stellar winds in the galactic centre

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

Producción científica: Contribución a una revista › Artículo de la conferencia › revisión exhaustiva

1 Cita (Scopus)

Resumen

Sgr A* is identi ed with the MBH-3.5×10⁶M super-massive black hole (SMBH) at the centre of our Galaxy. By virtue of its proximity, Sgr A* may play a key role in the understanding of Active Galactic Nuclei (AGN). Indeed, this is the only AGN where observations detail the origin of the gas in the vicinity of the SMBH. This information is absolutely necessary for the accretion problem to be modelled self-consistently.

Idioma original	Inglés
Páginas (desde-hasta)	139-140
Número de páginas	2
Publicación	Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
Volumen	26
Estado	Publicada - 2006
Publicado de forma externa	Sí
Evento	XI IAU Regional Latin American Meeting of Astronomy, LARIM2005 - Pucon, Chile Duración: 12 dic 2005 → 16 dic 2005

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@article{b9b6f1ced93f4f6cad82ed3d0624f01a,

title = "Accretion of stellar winds in the galactic centre",

abstract = "Sgr A* is identi ed with the MBH-3.5×106M super-massive black hole (SMBH) at the centre of our Galaxy. By virtue of its proximity, Sgr A* may play a key role in the understanding of Active Galactic Nuclei (AGN). Indeed, this is the only AGN where observations detail the origin of the gas in the vicinity of the SMBH. This information is absolutely necessary for the accretion problem to be modelled self-consistently.",

keywords = "Accretion, Accretion discs, Galaxy: Center, Stars: Winds, Out- flows",

author = "J. Cuadra and S. Nayakshin and V. Springel and \{Di Matteo\}, T.",

year = "2006",

language = "English",

volume = "26",

pages = "139--140",

journal = "Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias",

issn = "1405-2059",

publisher = "Universidad Nacional Autonoma de Mexico",

note = "XI IAU Regional Latin American Meeting of Astronomy, LARIM2005 ; Conference date: 12-12-2005 Through 16-12-2005",

}

TY - JOUR

T1 - Accretion of stellar winds in the galactic centre

AU - Cuadra, J.

AU - Nayakshin, S.

AU - Springel, V.

AU - Di Matteo, T.

PY - 2006

Y1 - 2006

N2 - Sgr A* is identi ed with the MBH-3.5×106M super-massive black hole (SMBH) at the centre of our Galaxy. By virtue of its proximity, Sgr A* may play a key role in the understanding of Active Galactic Nuclei (AGN). Indeed, this is the only AGN where observations detail the origin of the gas in the vicinity of the SMBH. This information is absolutely necessary for the accretion problem to be modelled self-consistently.

AB - Sgr A* is identi ed with the MBH-3.5×106M super-massive black hole (SMBH) at the centre of our Galaxy. By virtue of its proximity, Sgr A* may play a key role in the understanding of Active Galactic Nuclei (AGN). Indeed, this is the only AGN where observations detail the origin of the gas in the vicinity of the SMBH. This information is absolutely necessary for the accretion problem to be modelled self-consistently.

KW - Accretion, Accretion discs

KW - Galaxy: Center

KW - Stars: Winds, Out- flows

UR - https://www.scopus.com/pages/publications/70649095949

M3 - Conference article

AN - SCOPUS:70649095949

SN - 1405-2059

VL - 26

SP - 139

EP - 140

JO - Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

JF - Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

T2 - XI IAU Regional Latin American Meeting of Astronomy, LARIM2005

Y2 - 12 December 2005 through 16 December 2005

ER -

Accretion of stellar winds in the galactic centre

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