EXTENDED X-RAY EMISSION FROM A QUASAR-DRIVEN SUPERBUBBLE
Author(s): Greene, Jenny E.; Pooley, David; Zakamska, Nadia L; Comerford, Julia M; Sun, Ai-Lei
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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Greene, Jenny E. | - |
| dc.contributor.author | Pooley, David | - |
| dc.contributor.author | Zakamska, Nadia L | - |
| dc.contributor.author | Comerford, Julia M | - |
| dc.contributor.author | Sun, Ai-Lei | - |
| dc.date.accessioned | 2019-10-28T15:41:38Z | - |
| dc.date.available | 2019-10-28T15:41:38Z | - |
| dc.date.issued | 2014-06-10 | en_US |
| dc.identifier.citation | Greene, Jenny E, Pooley, David, Zakamska, Nadia L, Comerford, Julia M, Sun, Ai-Lei. (2014). EXTENDED X-RAY EMISSION FROM A QUASAR-DRIVEN SUPERBUBBLE. ASTROPHYSICAL JOURNAL, 788 (10.1088/0004-637X/788/1/54 | en_US |
| dc.identifier.issn | 0004-637X | - |
| dc.identifier.uri | http://arks.princeton.edu/ark:/88435/pr1h15b | - |
| dc.description.abstract | We present observations of extended, 20 kpc scale soft X-ray gas around a luminous obscured quasar hosted by an ultraluminous infrared galaxy caught in the midst of a major merger. The extended X-ray emission is well fit as a thermal gas with a temperature of kT approximate to 280 eV and a luminosity of L-X approximate to 10(42) erg s(-1) and is spatially coincident with a known ionized gas outflow. Based on the X-ray luminosity, a factor of similar to 10 fainter than the [O III] emission, we conclude that the X-ray emission is either dominated by photoionization, or by shocked emission from cloud surfaces in a hot quasar-driven wind. | en_US |
| dc.language.iso | en_US | en_US |
| dc.relation | https://ui.adsabs.harvard.edu/abs/2014ApJ...788...54G/abstract | en_US |
| dc.relation.ispartof | ASTROPHYSICAL JOURNAL | en_US |
| dc.rights | Final published version. Article is made available in OAR by the publisher's permission or policy. | en_US |
| dc.title | EXTENDED X-RAY EMISSION FROM A QUASAR-DRIVEN SUPERBUBBLE | en_US |
| dc.type | Journal Article | en_US |
| dc.identifier.doi | doi:10.1088/0004-637X/788/1/54 | - |
| dc.date.eissued | 2014-05-21 | en_US |
| dc.identifier.eissn | 1538-4357 | - |
| pu.type.symplectic | http://www.symplectic.co.uk/publications/atom-terms/1.0/journal-article | en_US |
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