Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..235f&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
Stellar Envelopes: Mass Loss
Scientific paper
We report the detection of CO J=1-0 of the circumstellar envelope of OH
26.5+0.6. From modelling both the dust and CO, we deduce that the
envelope structure is as followed: a superwind with a mass loss rate of
5×10-4 Msolar yr-1 surrounded by
a tenuous wind of 10-6 Msolar yr-1.
Campbell M. T.
Fong Dave
Justtanont Kay
Meixner Matthew
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