A Strong Flare of the H2O Maser in Sagittarius B2(M)

Details A Strong Flare of the H2O Maser in Sagittarius B2(M) A Strong Flare of the H2O Maser in Sagittarius B2(M)

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005arep...49..777r&link_type=abstract

Astronomy Reports, vol. 49, Issue 10, p.777-782

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Results of a study of a strong flare of H2O maser emission in the star-forming region Sgr B2(M) in 2004 are reported. The observations were carried out on the 22-m radio telescope of the Pushchino Radio Astronomy Observatory. The main emission, with its flux density reaching 3800 Jy, was concentrated in a narrow radial-velocity interval (about 3 km/s) and was most likely associated with the compact group r, while the emission at V LSR > 64 km/s came from group q. After 1994, the variations of the H2O maser emission in Sgr B2(M) became cyclic with a mean period of 3 years.

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