Three-dimensional simulations of a starburst wind

Jackie L. Cooper; Geoffrey V. Bicknell; Ralph S. Sutherland; Joss Bland-Hawthorn

doi:10.1007/s10509-007-9526-4

Three-dimensional simulations of a starburst wind

Jackie L. Cooper^*, Geoffrey V. Bicknell, Ralph S. Sutherland, Joss Bland-Hawthorn

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

5 Citations (Scopus)

Abstract

In order to better understand the formation of a starburst-driven wind, we have performed a series of three-dimensional hydrodynamical simulations in an inhomogeneous interstellar medium. We present the results of these simulations, which provide new insights into the formation of the optical filaments and the origin of the soft X-ray emission.

Original language	English
Pages (from-to)	99-103
Number of pages	5
Journal	Astrophysics and Space Science
Volume	311
Issue number	1-3
DOIs	https://doi.org/10.1007/s10509-007-9526-4
Publication status	Published - Oct 2007

Access to Document

10.1007/s10509-007-9526-4

Cite this

@article{914e291eb7684cd58f9fcb830b76437a,

title = "Three-dimensional simulations of a starburst wind",

abstract = "In order to better understand the formation of a starburst-driven wind, we have performed a series of three-dimensional hydrodynamical simulations in an inhomogeneous interstellar medium. We present the results of these simulations, which provide new insights into the formation of the optical filaments and the origin of the soft X-ray emission.",

keywords = "Galaxies: starburst, Hydrodynamics, ISM: jets \& outflows, Method: numerical",

author = "Cooper, \{Jackie L.\} and Bicknell, \{Geoffrey V.\} and Sutherland, \{Ralph S.\} and Joss Bland-Hawthorn",

year = "2007",

month = oct,

doi = "10.1007/s10509-007-9526-4",

language = "English",

volume = "311",

pages = "99--103",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

publisher = "Springer Netherlands",

number = "1-3",

}

TY - JOUR

T1 - Three-dimensional simulations of a starburst wind

AU - Cooper, Jackie L.

AU - Bicknell, Geoffrey V.

AU - Sutherland, Ralph S.

AU - Bland-Hawthorn, Joss

PY - 2007/10

Y1 - 2007/10

N2 - In order to better understand the formation of a starburst-driven wind, we have performed a series of three-dimensional hydrodynamical simulations in an inhomogeneous interstellar medium. We present the results of these simulations, which provide new insights into the formation of the optical filaments and the origin of the soft X-ray emission.

AB - In order to better understand the formation of a starburst-driven wind, we have performed a series of three-dimensional hydrodynamical simulations in an inhomogeneous interstellar medium. We present the results of these simulations, which provide new insights into the formation of the optical filaments and the origin of the soft X-ray emission.

KW - Galaxies: starburst

KW - Hydrodynamics

KW - ISM: jets & outflows

KW - Method: numerical

UR - https://www.scopus.com/pages/publications/35248871569

U2 - 10.1007/s10509-007-9526-4

DO - 10.1007/s10509-007-9526-4

M3 - Article

SN - 0004-640X

VL - 311

SP - 99

EP - 103

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1-3

ER -

Three-dimensional simulations of a starburst wind

Abstract

Access to Document

Other files and links

Fingerprint

Cite this