A study of OH and H2O masers in the circumstellar envelopes around Miras

Details A study of OH and H2O masers in the circumstellar envelopes around Miras A study of OH and H2O masers in the circumstellar envelopes around Miras

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..237m&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Oh And Water Masers, Evn/Global Vlbi And Merlin, Miras

Scientific paper

We study the mass loss phenomenon which is though to be generally seen in the evolution of late type stars. We are using radio interferometry European VLBI Network (EVN) and Multi-Element Radio Lined Network (MERLIN) to study maser emission from gas molecules of H2O and OH. This enable us to obtain 10-30 mas resolution images of mass loss in AGB stars.

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