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HIFI Survey of Emission-Line Galaxies: recent Results on the Nuclear Superbubble of NGC 3079

Published online by Cambridge University Press:  12 April 2016

S. Veilleux  and
G. Cecil
S. Veilleux
Affiliation:
Kitt Peak National Observatory, NOAO, Tucson, AZ 85726-6732, USA
G. Cecil
Affiliation:
Physics & Astronomy Dept., University of North Carolina, CB# 3255, Chapel Hill, NC 27599-3255, USA

Abstract

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The Hawaii Imaging Fabry-Perot Interferometer (HIFI) was used to produce a large data cube of the edge-on SBc galaxy NGC 3079 covering Hα + [NII] λλ6548, 6583. The complete two-dimensional coverage of the Fabry-Perot data allowed us to derive the general flow pattern of the nuclear gas that constitutes the energetic superbubble.

Type
2. The Fabry-Perot Spectrometer and its Applications
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 113 - 117
Copyright
Copyright © Astronomical Society of the Pacific 1995

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