Stellar-opacity calculations, 1: Lecture 2

Details Stellar-opacity calculations, 1: Lecture 2 Stellar-opacity calculations, 1: Lecture 2

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983swis.confr..21c&link_type=abstract

Presented at the Swiss Soc. of Astrophys. and Astronomy Conf., Saas Fee, Switzerland, 21-26 Mar. 1983

Astronomy and Astrophysics

Astronomy

Chemical Composition, Energy Transfer, Equations Of State, Nuclear Fusion, Mathematical Models, Temperature Gradients

Scientific paper

Stellar structure, evolution, stability, and pulsation or explosion were studied and it is noted that three very vital pieces of physical information are needed. It is assumed that the composition is known from observations of assumption. To construct a model of a star the following information is needed: the nuclear generation rates which give the luminosity the star emits and the pressure and energy equation of state which determines the flow of radiation through the star. The equation of state and opacity are discussed.

Affiliated with

Also associated with

No associations

Rating

Stellar-opacity calculations, 1: Lecture 2 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-opacity calculations, 1: Lecture 2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar-opacity calculations, 1: Lecture 2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1471208