The H2O masers in IC 10SE

Details The H2O masers in IC 10SE The H2O masers in IC 10SE

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...424l..33b&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 424, no. 1, p. L33-L36

Astronomy and Astrophysics

Astronomy

13

Dwarf Galaxies, Emission Spectra, Extragalactic Radio Sources, Masers, Radio Spectra, Star Formation, Time Measurement, Astronomical Observatories, Flux Density, Infrared Astronomy Satellite, Line Of Sight, Luminosity, Radial Velocity, Very Long Base Interferometry

Scientific paper

The H2O megamaser in IC 10SE has been observed at roughly monthly intervals using the Haystack Observatory from 1986 until 1993 as part of a monitoring program of galaxies with strong water masers. The IC 10SE maser features show strong variability in line strength, line velocity, and line width. An outburst of a single feature at -324 km/s with a flux density increase of 400 lasts for about 1 year. The characteristics of the features support unsaturated masering and amplification of background radio continuum.

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