On the post-asymptotic giant branch model for the far-ultraviolet emission in elliptical galaxies

Details On the post-asymptotic giant branch model for the far-ultraviolet emission in elliptical galaxies On the post-asymptotic giant branch model for the far-ultraviolet emission in elliptical galaxies

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339..889b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 15, 1989, p. 889-903. Research supported by CNR.

Astronomy and Astrophysics

Astronomy

30

Astronomical Models, Asymptotic Giant Branch Stars, Elliptical Galaxies, Far Ultraviolet Radiation, Galactic Radiation, Stellar Evolution, Chemical Composition, Emission Spectra, Globular Clusters, Metallicity, Stellar Envelopes, Stellar Mass, Ultraviolet Astronomy

Scientific paper

New calculations of evolutionary sequences for low- and
intermediate-mass stars are used to study the post-asymptotic giant
branch model. An attempt is made to show that flaws and inconsistencies
found previously have no reason to occur. A solution is proposed for the
FUV emission in elliptical galaxies which is internally consistent.

Affiliated with

Also associated with

No associations

Rating

On the post-asymptotic giant branch model for the far-ultraviolet emission in elliptical galaxies 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 On the post-asymptotic giant branch model for the far-ultraviolet emission in elliptical galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the post-asymptotic giant branch model for the far-ultraviolet emission in elliptical galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1735779