The fate of gas in cluster galaxies: Winds and stripping

Eelco van Kampen; Wilfried Domainko; Olfgang Kapferer; Stefan Kimeswenger; Thomas Kronberger; Magdalena Mair; Rainer Moll; Sabine Schindler; Maximilian Ruffert; Otonyo Mangete; Chris Rimes

doi:10.1016/j.newar.2006.11.012

The fate of gas in cluster galaxies: Winds and stripping

Eelco van Kampen, Wilfried Domainko, Olfgang Kapferer, Stefan Kimeswenger, Thomas Kronberger, Magdalena Mair, Rainer Moll, Sabine Schindler, Maximilian Ruffert, Otonyo Mangete, Chris Rimes

School of Mathematics

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

Abstract

The fate of gas in cluster galaxies through the dynamical processes of ram-pressure stripping and winds is modelled using a combined N-body, phenomenological and hydrodynamical approach. This allows us to model the interaction between cluster galaxies and the intra-cluster medium, and study the consequences of this interaction on the metallicity of the hot cluster gas as well as the properties of the cluster galaxies. We summarize our results for the ICM metallicity, and discuss a first attempt to improve the predictions for the properties of cluster galaxies. (c) 2006 Elsevier B.V. All rights reserved.

Original language	English
Pages (from-to)	84-86
Number of pages	3
Journal	New Astronomy Reviews
Volume	51
Issue number	1-2
DOIs	https://doi.org/10.1016/j.newar.2006.11.012
Publication status	Published - Feb 2007

Keywords

SIMULATIONS
ENRICHMENT
STAR

Access to Document

10.1016/j.newar.2006.11.012

Cite this

@article{2f8c55c059e54d5eac9ff1d178f0f626,

title = "The fate of gas in cluster galaxies: Winds and stripping",

abstract = "The fate of gas in cluster galaxies through the dynamical processes of ram-pressure stripping and winds is modelled using a combined N-body, phenomenological and hydrodynamical approach. This allows us to model the interaction between cluster galaxies and the intra-cluster medium, and study the consequences of this interaction on the metallicity of the hot cluster gas as well as the properties of the cluster galaxies. We summarize our results for the ICM metallicity, and discuss a first attempt to improve the predictions for the properties of cluster galaxies. (c) 2006 Elsevier B.V. All rights reserved.",

keywords = "SIMULATIONS, ENRICHMENT, STAR",

author = "{van Kampen}, Eelco and Wilfried Domainko and Olfgang Kapferer and Stefan Kimeswenger and Thomas Kronberger and Magdalena Mair and Rainer Moll and Sabine Schindler and Maximilian Ruffert and Otonyo Mangete and Chris Rimes",

year = "2007",

month = feb,

doi = "10.1016/j.newar.2006.11.012",

language = "English",

volume = "51",

pages = "84--86",

journal = "New Astronomy Reviews",

issn = "1387-6473",

publisher = "Elsevier",

number = "1-2",

}

The fate of gas in cluster galaxies: Winds and stripping. / van Kampen, Eelco; Domainko, Wilfried; Kapferer, Olfgang; Kimeswenger, Stefan; Kronberger, Thomas; Mair, Magdalena; Moll, Rainer; Schindler, Sabine; Ruffert, Maximilian; Mangete, Otonyo; Rimes, Chris.

In: New Astronomy Reviews, Vol. 51, No. 1-2, 02.2007, p. 84-86.

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

TY - JOUR

T1 - The fate of gas in cluster galaxies: Winds and stripping

AU - van Kampen, Eelco

AU - Domainko, Wilfried

AU - Kapferer, Olfgang

AU - Kimeswenger, Stefan

AU - Kronberger, Thomas

AU - Mair, Magdalena

AU - Moll, Rainer

AU - Schindler, Sabine

AU - Ruffert, Maximilian

AU - Mangete, Otonyo

AU - Rimes, Chris

PY - 2007/2

Y1 - 2007/2

N2 - The fate of gas in cluster galaxies through the dynamical processes of ram-pressure stripping and winds is modelled using a combined N-body, phenomenological and hydrodynamical approach. This allows us to model the interaction between cluster galaxies and the intra-cluster medium, and study the consequences of this interaction on the metallicity of the hot cluster gas as well as the properties of the cluster galaxies. We summarize our results for the ICM metallicity, and discuss a first attempt to improve the predictions for the properties of cluster galaxies. (c) 2006 Elsevier B.V. All rights reserved.

AB - The fate of gas in cluster galaxies through the dynamical processes of ram-pressure stripping and winds is modelled using a combined N-body, phenomenological and hydrodynamical approach. This allows us to model the interaction between cluster galaxies and the intra-cluster medium, and study the consequences of this interaction on the metallicity of the hot cluster gas as well as the properties of the cluster galaxies. We summarize our results for the ICM metallicity, and discuss a first attempt to improve the predictions for the properties of cluster galaxies. (c) 2006 Elsevier B.V. All rights reserved.

KW - SIMULATIONS

KW - ENRICHMENT

KW - STAR

U2 - 10.1016/j.newar.2006.11.012

DO - 10.1016/j.newar.2006.11.012

M3 - Article

VL - 51

SP - 84

EP - 86

JO - New Astronomy Reviews

JF - New Astronomy Reviews

SN - 1387-6473

IS - 1-2

ER -