The gas shells of RS Puppis

Details The gas shells of RS Puppis The gas shells of RS Puppis

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988iraj...18..249w&link_type=abstract

(Astronomocal Science Group of Ireland, Meeting, University College, Cork, Republic of Ireland, Mar. 31, 1988) Irish Astronomica

Astronomy and Astrophysics

Astronomy

Cepheid Variables, Nebulae, Stellar Envelopes, Cosmic Dust, Infrared Astronomy Satellite, Photosphere, Stellar Models, Stellar Temperature

Scientific paper

Recent optical, near-infrared, and IRAS observations of the nebular structure around the 41-day Cepheid RS Puppis are reviewed. The structure is found to display successive shells which, at any rate in the optical range, mirror the light variations of the central star. Expanding shell models were used by Deasy (1988) to obtain mass values of about 0.045, 0.073, and 0.044 solar massses for the three principal shells of RS Puppis.

Affiliated with

Also associated with

No associations

Rating

The gas shells of RS Puppis 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 The gas shells of RS Puppis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The gas shells of RS Puppis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-913967