Kinematic Interpretation of the Centaurus A Absorption‐Line System
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/516/i=2/a=769/pdf
Reference47 articles.
1. Detection of C3H2 emission in the radio galaxy centaurus A (= NGC 5128)
2. The structure and kinematics of the ionized gas within NGC 5128 (Cen A) – I. TAURUS observations
3. Wind from a starburst galaxy nucleus
4. Distance of M83 and of the Centaurus group
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1. ALMA Observations of the Physical and Chemical Conditions in Centaurus A;The Astrophysical Journal;2017-12-14
2. Disentangling the Circumnuclear Environs of Centaurus A. III. An Inner Molecular Ring, Nuclear Shocks, and the CO to Warm H2Interface;The Astrophysical Journal;2017-07-13
3. DISENTANGLING THE CIRCUMNUCLEAR ENVIRONS OF CENTAURUS A. II. ON THE NATURE OF THE BROAD ABSORPTION LINE;The Astrophysical Journal;2010-08-12
4. The Many Faces of the Gas in Centaurus A (NGC 5128);Publications of the Astronomical Society of Australia;2010
5. HCO+AND HCNJ= 3-2 ABSORPTION TOWARD THE CENTER OF CENTAURUS A;The Astrophysical Journal;2009-04-15
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