Stellar Evolution

Details Stellar Evolution Stellar Evolution

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002eaa..booke1879c&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 1879. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Stars, Stellar Models And Concepts

Scientific paper

Stars evolve because they lose energy through radiation from their hot surfaces. As a result, there is a general tendency for the star to contract under gravity. This is partly stopped by the release of energy from nuclear reactions. However, once the nuclear fuel is exhausted, gravity gets the upper hand and the star ends its life as a compact object: a white dwarf, a neutron star or a black hol...

Affiliated with

Also associated with

No associations

Rating

Stellar Evolution 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 Stellar Evolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar Evolution will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1089174