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HI and OH Absorption of the Nuclear Region of NGC 3079

Published online by Cambridge University Press:  13 May 2016

S. Sawada-Satoh ,
M. Inoue ,
K.M. Shibata ,
S. Kameno ,
N. Nakai ,
V. Migenes  and
P.J. Diamond
S. Sawada-Satoh
Affiliation:
NAO, Mitaka, Tokyo, 181-8588 JAPAN
M. Inoue
Affiliation:
NAO, Mitaka, Tokyo, 181-8588 JAPAN
K.M. Shibata
Affiliation:
NAO, Mitaka, Tokyo, 181-8588 JAPAN
S. Kameno
Affiliation:
NAO, Mitaka, Tokyo, 181-8588 JAPAN
N. Nakai
Affiliation:
NAO, Mitaka, Tokyo, 181-8588 JAPAN
V. Migenes
Affiliation:
Universidad de Guanajuato, Guanajuato, CP 36000, MEXICO
P.J. Diamond
Affiliation:
JBO, Jodrell Bank, Macclesfield, Cheshire, SK11 9DL U.K.

Abstract

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We conducted an observation of weak HI and OH absorption features in the parsec-scale nuclear region of NGC 3079 using a global VLBI network; the VLBA, the VLA and the Green Bank 43-m telescope of NRAO. One mas corresponds to 0.076 pc in NGC 3079.

Type
The Inner Regions of Galaxies
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 196 - 197
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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