Observational study on extragalactic H2O megamaser sources and associated molecular emission lines

Details Observational study on extragalactic H2O megamaser sources and associated molecular emission lines Observational study on extragalactic H2O megamaser sources and associated molecular emission lines

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pabei..20..256y&link_type=abstract

Progress in Astronomy (ISSN 1000-8349), Vol. 20, No. 3, p. 256 - 264 (2002)

Astronomy and Astrophysics

Astronomy

Agn, Extragalactic Water Megamaser, Molecular Emission Line

Scientific paper

Since the first extragalactic H2O megamaser source toward the active galactic nuclei NGC 4945 was discovered, 19 sources have been found. The observational study of extragalactic H2O megamaser sources and molecular emission lines associated with AGNs is a very efficient tool to investigate characteristics of central sources in AGNs and circumnuclear tori of gas and dust. Current researches of searching, observation and theory on extragalactic H2O megamaser sources and associated molecular emission lines are mainly reviewed in this paper.

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