Chemistry in anisotropic asymptotic giant branch winds

Details Chemistry in anisotropic asymptotic giant branch winds Chemistry in anisotropic asymptotic giant branch winds

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.282l..21h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 282, Issue 1, pp. L21-L25.

Astronomy and Astrophysics

Astronomy

1

Molecular Processes, Stars: Agb And Post-Agb, Circumstellar Matter, Stars: Individual: Irc+10216

Scientific paper

We have constructed a model for chemistry in the outflow of an asymptotic giant branch (AGB) star, using a spheroidal anisotropy in density, after that used by Jura. The predicted distributions of a selection of representative species are shown, and it is suggested that the abundance distributions observed by interferometry in IRC+10216 may be the result of directional variation in outflow velocity.

Affiliated with

Also associated with

No associations

Rating

Chemistry in anisotropic asymptotic giant branch winds 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 Chemistry in anisotropic asymptotic giant branch winds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemistry in anisotropic asymptotic giant branch winds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-994837