Clump formation through colliding stellar winds in the Galactic Centre

D. Calderón; J. Cuadra; A. Ballone; M. Schartmann; A. Burkert; J. Prieto; S. Gillessen

doi:10.1017/S1743921316012011

Clump formation through colliding stellar winds in the Galactic Centre

D. Calderón, J. Cuadra, A. Ballone, M. Schartmann, A. Burkert, J. Prieto, S. Gillessen

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

Resumen

We study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising sources being compact massive binaries, such as IRS 16SW.

Idioma original	Inglés
Páginas (desde-hasta)	204-205
Número de páginas	2
Publicación	Proceedings of the International Astronomical Union
Volumen	11
DOI	https://doi.org/10.1017/S1743921316012011
Estado	Publicada - 2016
Publicado de forma externa	Sí

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title = "Clump formation through colliding stellar winds in the Galactic Centre",

abstract = "We study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising sources being compact massive binaries, such as IRS 16SW.",

keywords = "hydrodynamics - instabilities - stars: winds, outflows - Galaxy: centre",

author = "D. Calder{\'o}n and J. Cuadra and A. Ballone and M. Schartmann and A. Burkert and J. Prieto and S. Gillessen",

note = "Publisher Copyright: {\textcopyright} 2017 International Astronomical Union.",

year = "2016",

doi = "10.1017/S1743921316012011",

language = "English",

volume = "11",

pages = "204--205",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

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T1 - Clump formation through colliding stellar winds in the Galactic Centre

AU - Calderón, D.

AU - Cuadra, J.

AU - Ballone, A.

AU - Schartmann, M.

AU - Burkert, A.

AU - Prieto, J.

AU - Gillessen, S.

PY - 2016

Y1 - 2016

N2 - We study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising sources being compact massive binaries, such as IRS 16SW.

AB - We study the process of clump formation from hydrodynamic instabilities in stellar wind collisions, using analytical and numerical techniques. We show that the cloud G2 in the Galactic Centre could have been formed in this way, with the most promising sources being compact massive binaries, such as IRS 16SW.

KW - hydrodynamics - instabilities - stars: winds

KW - outflows - Galaxy: centre

UR - http://www.scopus.com/inward/record.url?scp=85012297946&partnerID=8YFLogxK

U2 - 10.1017/S1743921316012011

DO - 10.1017/S1743921316012011

M3 - Article

AN - SCOPUS:85012297946

SN - 1743-9213

VL - 11

SP - 204

EP - 205

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

ER -

Clump formation through colliding stellar winds in the Galactic Centre

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