Radio and infrared observations of circumstellar envelopes - The progress since 1984

Details Radio and infrared observations of circumstellar envelopes - The progress since 1984 Radio and infrared observations of circumstellar envelopes - The progress since 1984

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ssrv...47..145o&link_type=abstract

Space Science Reviews (ISSN 0038-6308), vol. 47, no. 1-2, 1988, p. 145-174. Research supported by Chalmers Tekniska Hogskola and

Astronomy and Astrophysics

Astronomy

16

Asymptotic Giant Branch Stars, Infrared Astronomy, Interstellar Chemistry, Interstellar Matter, Radio Astronomy, Stellar Envelopes, Color-Color Diagram, H I Regions, Hydroxyl Emission, Infrared Astronomy Satellite, Planetary Nebulae, Stellar Mass Ejection

Scientific paper

The observational achievements at radio and infrared wavelengths since 1984 concerning the circumstellar envelopes of evolved stars are summarized. Knowledge of late stellar evolution during the asymptotic giant branch phase and the transition to the planetary nebula stage is discussed as well as the properties of gas/dust envelopes formed by stellar mass loss. New circumstellar molecules are considered as well as spectral scans, vibrationally excited lines, isotopic species, the time variability of thermal emission, and spatial structure.

Affiliated with

Also associated with

No associations

Rating

Radio and infrared observations of circumstellar envelopes - The progress since 1984 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 Radio and infrared observations of circumstellar envelopes - The progress since 1984, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio and infrared observations of circumstellar envelopes - The progress since 1984 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1693392