An evolutionary sequence of models of planetary nebulae

Details An evolutionary sequence of models of planetary nebulae An evolutionary sequence of models of planetary nebulae

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..332v&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, Mar.-Apr. 1983, p. 332-339) Soviet Astronomy (ISSN 0038-5301), vol. 27, Mar.-Apr. 1983, p. 1

Astronomy and Astrophysics

Astronomy

4

Astronomical Models, Planetary Nebulae, Stellar Evolution, Emission Spectra, H Beta Line, Mass Distribution, Stellar Luminosity, Stellar Temperature

Scientific paper

Evolutionary sequences of models of planetary nebulae of different masses are calculated. The calculated line intensities are compared with the observed ones using an identically defined parameter, the 'reduced size of the nebula'. Schonberner's (1979, 1981) evolutionary tracks for the central stars of nebulae lead to results consistent with observational data.

Affiliated with

Also associated with

No associations

Rating

An evolutionary sequence of models of planetary nebulae 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 An evolutionary sequence of models of planetary nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An evolutionary sequence of models of planetary nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1234006