From the AGB to the PN Phase with the Plateau de Bure Interferometer

Details From the AGB to the PN Phase with the Plateau de Bure Interferometer From the AGB to the PN Phase with the Plateau de Bure Interferometer

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313..314c&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

3

Scientific paper

In order to understand the origin of the asymmetries and substructures observed in planetary nebulae, it is necessary to improve our knowledge on their progenitors, the circumstellar envelopes (CSEs) of asymptotic giant branch (AGB) stars and proto-planetary nebulae (PPNe). These nebulae are mainly composed of cool molecular gas and therefore they are accessible to mm-observations. The Plateau de Bure interferometer has played an important role in the advance of our understanding of these objects in the last 10 yr.

Affiliated with

Also associated with

No associations

Rating

From the AGB to the PN Phase with the Plateau de Bure Interferometer 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 From the AGB to the PN Phase with the Plateau de Bure Interferometer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and From the AGB to the PN Phase with the Plateau de Bure Interferometer will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1076539