VLBA observations of the υ = 1 and 2 SiO J = 1-0 maser emissions in VY CMa

Details VLBA observations of the υ = 1 and 2 SiO J = 1-0 maser emissions in VY CMa VLBA observations of the υ = 1 and 2 SiO J = 1-0 maser emissions in VY CMa

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..303m&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

5

Sio Masers, Vlba, Vy Cma

Scientific paper

We performed VLBA observations of SiO masers in VY CMa. While some maser
spots exist that have no counterpart in another line, the difference of
distributions of the SiO J=1-0 maser emissions in υ=1 and υ=2
states is within 0.2 mas (= 0.3 AU at the distance of 1.5 kpc) in
average.

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