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An atlas of extragalactic water vapor masers

Published online by Cambridge University Press:  01 March 2007

J. Braatz ,
P. Kondratko ,
L. Greenhill ,
J. Condon ,
C. Henkel ,
N. Gugliucci ,
L. Hao ,
M. Reid ,
J. Moran  and
K.-Y. Lo
J. Braatz
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA email: [email protected]
P. Kondratko
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
L. Greenhill
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
J. Condon
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA email: [email protected]
C. Henkel
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
N. Gugliucci
Affiliation:
Dept. of Astronomy, University of Virginia, Charlottesville, VA, USA
L. Hao
Affiliation:
Dept. of Astronomy, Cornell University, Ithaca, NY, USA
M. Reid
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
J. Moran
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
K.-Y. Lo
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA email: [email protected]
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Abstract

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We present an atlas of extragalactic water vapor masers. As of 2007, one hundred galaxies have been detected as sources of water vapor maser emission, two thirds of them discovered since 2003. Extragalactic water masers fall in at least three categories: those associated with nuclear jets or winds, those in starbursts or star-forming regions, and those in AGN accretion disks. While all maser systems offer the possibility of unique investigations into their physical environments, it is the disk masers that have been most aggressively sought because of their potential for use as precision distance indicators. Type 2 Seyfert and LINER galaxies are hosts to such disk masers. Insingle-dish spectra, disk masers are often revealed by the presence of high-velocity emission features (defined roughly by having anomalous velocities in excess of 200 km s−1). About one third of the extragalactic water masers detected to date show evidence of disk origin. Only a few galaxies are currently identified as jet-type or star-forming type. The remaining systems show only a few narrow doppler components, usually near the systemic velocity, and are difficult to categorize. These unclassified systems are detected toward AGNs and are also possibly associated with disks or winds near the nucleus. Detection rates in large maser surveys are typically 5% or less, but the observing efficiency and sensitivity of the Green Bank Telescope (GBT) allow for short integration times (typically 10 minutes to detect a narrow 30 mJy line) so many galaxies can be searched. Recently, GBT surveys targeting type 2 Seyfert galaxies identified by the SDSS have been the most productive, identifying 17 systems in surveys observed during 2006.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 402 - 403
Copyright
Copyright © International Astronomical Union 2008