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Gemini GMOS and WHT SAURON integral-field spectrograph observations of the AGN-driven outflow in NGC 1266

Abstract:

We use the Spectrographic Areal Unit for Research on Optical Nebulae and Gemini Multi-Object Spectrograph integral-field spectrographs to observe the active galactic nucleus (AGN) powered outflow in NGC1266. This unusual galaxy is relatively nearby (D = 30Mpc), allowing us to investigate the process of AGN feedback in action. We present maps of the kinematics and line strengths of the ionized gas emission lines Hα, Hβ, [Oiii], [Oi], [Nii] and [Sii], and report on the detection of sodium D abs...

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Publication status:
Published

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Authors


Krajnovic, D More by this author
McDermid, RM More by this author
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Journal:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume:
426
Issue:
2
Pages:
1574-1590
Publication date:
2012-10-05
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:a3a4b191-284c-4071-b922-cfb9f39da26f
Source identifiers:
354633
Local pid:
pubs:354633

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