A comparison of the SiO masers in Orion KL with those of late type stars

Details A comparison of the SiO masers in Orion KL with those of late type stars A comparison of the SiO masers in Orion KL with those of late type stars

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..321m&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

Sio Masers, Vlba, Orion-Kl

Scientific paper

Using the VLBA, we observed the SiO J=1-0 masers lines at the v=1 and
v=2 states in the Orion KL. The spatial distribution of the Orion KL
shows no regularity in two lines, though supergiant VY CMa shows good
correlation. The environment where the SiO masers generate is different
between late type stars and star forming regions.

Affiliated with

Also associated with

No associations

Rating

A comparison of the SiO masers in Orion KL with those of late type stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A comparison of the SiO masers in Orion KL with those of late type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A comparison of the SiO masers in Orion KL with those of late type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-920713