The H_2O Maser Toward IRAS 06308+0402

Details The H_2O Maser Toward IRAS 06308+0402 The H_2O Maser Toward IRAS 06308+0402

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003astl...29..731p&link_type=abstract

Astronomy Letters, vol. 29, p. 731-736 (2003)

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We present the monitoring results for the H_2O maser toward the infrared source IRAS 06308+0402 associated with a dense cold molecular cloud. The observations were carried out with the 22-m radio telescope at the Pushchino Radio Astronomy Observatory (Russia) during 1992-2003. The H_2O maser was discovered in May 1992 (Pashchenko 1992) during a survey of IRAS sources associated with dense cold clouds with bipolar molecular outflows. The H_2O spectrum contains many emission features, suggesting the fragmentation of the envelope around a young star. The star has a low peculiar velocity relative to the CO molecular cloud (~2.2 km/s). We found a cyclic variability of the total maser flux with a period from 1.8 to 3.1 yr.

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