Heating of the intracluster medium by quasar outflows
We study the possibility of quasar outflows in clusters and groups of galaxies heating the intracluster gas in order to explain the recent observation of excess entropy in this gas. We show that radio galaxies alone cannot provide the energy required to explain the observations but the inclusion of...
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Published in | Journal of astrophysics and astronomy Vol. 23; no. 1-2; pp. 101 - 105 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Bangalore
Springer Nature B.V
01.03.2002
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Subjects | |
Online Access | Get full text |
ISSN | 0250-6335 0973-7758 |
DOI | 10.1007/BF02702472 |
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Abstract | We study the possibility of quasar outflows in clusters and groups of galaxies heating the intracluster gas in order to explain the recent observation of excess entropy in this gas. We show that radio galaxies alone cannot provide the energy required to explain the observations but the inclusion of Broad Absorption Line (BAL) outflows can do so, and that in this scenario most of the heating takes place at z 1-4, the "preheating" epoch being at a lower redshift for lower mass clusters. |
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AbstractList | We study the possibility of quasar outflows in clusters and groups of galaxies heating the intracluster gas in order to explain the recent observation of excess entropy in this gas. We show that radio galaxies alone cannot provide the energy required to explain the observations but the inclusion of Broad Absorption Line (BAL) outflows can do so, and that in this scenario most of the heating takes place at iz 1-4, the "preheating" epoch being at a lower redshift for lower mass clusters. We study the possibility of quasar outflows in clusters and groups of galaxies heating the intracluster gas in order to explain the recent observation of excess entropy in this gas. We show that radio galaxies alone cannot provide the energy required to explain the observations but the inclusion of Broad Absorption Line (BAL) outflows can do so, and that in this scenario most of the heating takes place at z 1-4, the "preheating" epoch being at a lower redshift for lower mass clusters. We study the possibility of quasar outflows in clusters and groups of galaxies heating the intracluster gas in order to explain the recent observation of excess entropy in this gas. We show that radio galaxies alone cannot provide the energy required to explain the observations but the inclusion of Broad Absorption Line (BAL) outflows can do so, and that in this scenario most of the heating takes place atz ∼ 1–4, the “preheating” epoch being at a lower redshift for lower mass clusters. We study the possibility of quasar outflows in clusters and groups of galaxies heating the intracluster gas in order to explain the recent observation of excess entropy in this gas. We show that radio galaxies alone cannot provide the energy required to explain the observations but the inclusion of Broad Absorption Line (BAL) outflows can do so, and that in this scenario most of the heating takes place atz 1-4, the "preheating" epoch being at a lower redshift for lower mass clusters.[PUBLICATION ABSTRACT] |
Author | Roychowdhury, Suparna Nath, Biman B. |
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Cites_doi | 10.1093/mnras/169.3.395 10.1046/j.1365-8711.2000.03380.x 10.1093/mnras/166.3.513 10.1086/321630 10.1086/170768 10.1086/177797 10.1038/16410 10.1093/mnras/262.3.627 10.1086/300353 10.1086/304400 10.1086/307604 10.1046/j.1365-8711.2000.03828.x 10.1046/j.1365-8711.2002.05389.x 10.1093/mnras/248.2.332 10.1086/318174 10.1086/306017 |
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SubjectTerms | Astrophysics Entropy Galactic clusters Galaxies Heating Outflow Quasars Radio galaxies Red shift |
Title | Heating of the intracluster medium by quasar outflows |
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