The Discovery of H2O Maser Emission in Seven AGN and at High Velocities in the Circinus Galaxy

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4 pages, including 2 figures. To appear in ApJ Letters Jan. 1, 2003 edition

Scientific paper

10.1086/367602

We report the discovery of H2O maser emission at 1.35 cm wavelength in seven active galactic nuclei (at distances up to <80 Mpc) during a survey conducted at the 70-m diameter antenna of the NASA Deep Space Network near Canberra, Australia. The detection rate was (approx.) 4%. Two of the maser sources are particularly interesting because they display satellite high-velocity emission lines, which are a signature of emission from the accretion disks of supermassive black holes when seen edge on. Three of the masers are coincident, to within uncertainties of 0.''2, with continuum emission sources we observed at about (lamda)1.3 cm. We also report the discovery of new spectral features in the Circinus galaxy H2O maser that broaden the known velocity range of emission therein by a factor of (approx.) 1.7. If the new spectral features originate in the Circinus accretion disk, then molecular material must survive at radii (approx.) 3 times smaller than had been believed previously [(approx.) 0.03 pc or (approx.) 2 x 105 Schwarzschild radii].

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The Discovery of H2O Maser Emission in Seven AGN and at High Velocities in the Circinus Galaxy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Discovery of H2O Maser Emission in Seven AGN and at High Velocities in the Circinus Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Discovery of H2O Maser Emission in Seven AGN and at High Velocities in the Circinus Galaxy will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-602337

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.