The results of ultra-rapid flux fluctuations monitoring in 2002-2009 for galactic sources of water-vapor maser emission at a wavelength of 1.35 cm

Details The results of ultra-rapid flux fluctuations monitoring in 2002-2009 for galactic sources of water-vapor maser emission at a wavelength of 1.35 cm The results of ultra-rapid flux fluctuations monitoring in 2002-2009 for galactic sources of water-vapor maser emission at a wavelength of 1.35 cm

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1206..346s&link_type=abstract

ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: Proceedings of the 4th Gamow International Conference on Astrophysics and Cosmology Afte

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Cyclotron Masers, Gravitational Waves, Radio Galaxies, Interstellar Masers, Gravitational Radiation, Magnetic Fields, And Other Observations, Radio Galaxies

Scientific paper

Results of a search for ultra rapid flux fluctuations of galactic sources of maser emission in the water-vapor line at a wavelength of 1.35 cm. An observational technique of a search for ultra rapid flux fluctuations has been developed. From 2002 to 2009 a number of observational sessions for about 40 maser sources have been carried out. Several of them have demonstrated such a variability. Possible mechanisms of the variability are discussed, among them internal processes within the sources themselves as well as external ones, including the theoretical possibility of a resonant effect of gravitational waves from galactic objects on the maser region. Clear evidence for the presence of such a variability has been found in several sources (Cep A, W43M3, W49N, W33B). This variability appears not permanently, but only certain states of particular H2O masers. In some sources (Ori A, W3 OH, W49N) demonstrated any variations by linear polarization of signal.

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