SiO Maser Emission in V838 Mon

Details SiO Maser Emission in V838 Mon SiO Maser Emission in V838 Mon

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..363...81d&link_type=abstract

The Nature of V838 Mon and its Light Echo ASP Conference Series, Vol. 363, Proceedings of the conference held 16-19 May, 2006 in

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Scientific paper

We present further radio observations of V838 Mon in the SiO and several other molecular lines after 2005 April. The detection of SiO masers in this object indicates that the star formed after eruption is indeed a cool mass-losing object with circumstellar masers. Further observations of SiO masers found a sudden increase within a few months and succeeding flattening of maser intensities, suggesting a sudden slow onset of mass-loss from the central star after the 2002 eruption. A detection of CO emission 30'' north of the star is also reported. A possible implication for stellar evolution in related objects is given.

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