INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES
In preparation for a study of their circumnuclear gas we have surveyed 60% of a complete sample of elliptical galaxies within 75 Mpc that are radio sources. Some 20% of our nuclear spectra have infrared emission lines, mostly Paschen lines, Brackett γ, and [Fe II]. We consider the influence of radio...
| Main Authors: | , , , , , , , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2012
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| _version_ | 1826274036138639360 |
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| author | Mould, J Reynolds, T Readhead, T Floyd, D Jannuzi, B Cotter, G Ferrarese, L Matthews, K Atlee, D Brown, M |
| author_facet | Mould, J Reynolds, T Readhead, T Floyd, D Jannuzi, B Cotter, G Ferrarese, L Matthews, K Atlee, D Brown, M |
| author_sort | Mould, J |
| collection | OXFORD |
| description | In preparation for a study of their circumnuclear gas we have surveyed 60% of a complete sample of elliptical galaxies within 75 Mpc that are radio sources. Some 20% of our nuclear spectra have infrared emission lines, mostly Paschen lines, Brackett γ, and [Fe II]. We consider the influence of radio power and black hole mass in relation to the spectra. Access to the spectra is provided here as a community resource. © 2012. The American Astronomical Society. All rights reserved.. |
| first_indexed | 2024-03-06T22:37:20Z |
| format | Journal article |
| id | oxford-uuid:5a585ce0-231a-4d19-ac0a-5e60c28a6873 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-06T22:37:20Z |
| publishDate | 2012 |
| record_format | dspace |
| spelling | oxford-uuid:5a585ce0-231a-4d19-ac0a-5e60c28a68732022-03-26T17:15:18ZINFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIESJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:5a585ce0-231a-4d19-ac0a-5e60c28a6873EnglishSymplectic Elements at Oxford2012Mould, JReynolds, TReadhead, TFloyd, DJannuzi, BCotter, GFerrarese, LMatthews, KAtlee, DBrown, MIn preparation for a study of their circumnuclear gas we have surveyed 60% of a complete sample of elliptical galaxies within 75 Mpc that are radio sources. Some 20% of our nuclear spectra have infrared emission lines, mostly Paschen lines, Brackett γ, and [Fe II]. We consider the influence of radio power and black hole mass in relation to the spectra. Access to the spectra is provided here as a community resource. © 2012. The American Astronomical Society. All rights reserved.. |
| spellingShingle | Mould, J Reynolds, T Readhead, T Floyd, D Jannuzi, B Cotter, G Ferrarese, L Matthews, K Atlee, D Brown, M INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES |
| title | INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES |
| title_full | INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES |
| title_fullStr | INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES |
| title_full_unstemmed | INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES |
| title_short | INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES |
| title_sort | infrared spectroscopy of nearby radio active elliptical galaxies |
| work_keys_str_mv | AT mouldj infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT reynoldst infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT readheadt infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT floydd infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT jannuzib infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT cotterg infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT ferraresel infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT matthewsk infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT atleed infraredspectroscopyofnearbyradioactiveellipticalgalaxies AT brownm infraredspectroscopyofnearbyradioactiveellipticalgalaxies |