Evolution of the double peak spectrum of the OH-1612 MHz maser on the asymptotic giant branch

Details Evolution of the double peak spectrum of the OH-1612 MHz maser on the asymptotic giant branch Evolution of the double peak spectrum of the OH-1612 MHz maser on the asymptotic giant branch

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991cha%26a..15..197s&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, June 1991, p. 197-206. Translation. NNSFC-supported research.

Astronomy and Astrophysics

Astrophysics

1

Asymptotic Giant Branch Stars, Interstellar Masers, Maser Outputs, Water Masers, Spectrum Analysis, Stellar Evolution, Stellar Mass Ejection

Scientific paper

Observations of asymptotic giant branch (AGB) stars associated with the OH 1612 MHz maser are used to study the evolution of the double-peak spectrum of the maser when the mass-loss rate of the AGB star (M) varies in time. The empirical relations between the OH emission range and M, and between the maser luminosity and M are reproduced. The model also indicates that the OH emission can last over 100-500 years after the termination of the AGB.

Affiliated with

Also associated with

No associations

Rating

Evolution of the double peak spectrum of the OH-1612 MHz maser on the asymptotic giant branch 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 Evolution of the double peak spectrum of the OH-1612 MHz maser on the asymptotic giant branch, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of the double peak spectrum of the OH-1612 MHz maser on the asymptotic giant branch will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1282501