Code for the computation of the structural and chemical evolution of stars

Details Code for the computation of the structural and chemical evolution of stars Code for the computation of the structural and chemical evolution of stars

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007asd..soft...34s&link_type=abstract

Astrophysics Software Database, CAU Kiel, Germany (http://www1.astrophysik.uni-kiel.de/asd/).

Astronomy and Astrophysics

Astrophysics

Fortran

Scientific paper

One dimensional hydrodynamic Lagrangian code, computing the evolution of stars of any metallicity in the mass range 0.1 to 60 Msun, from the pre-main sequence up to the final stages of the evolution. The code includes a self-consistent treatment of several dynamical processes : mass loss, accretion, atomic diffusion, transport of angular momentum and chemicals by rotation (2D treatment) and internal gravity waves, and the propagation of flames and shock waves .

Affiliated with

Also associated with

No associations

Rating

Code for the computation of the structural and chemical evolution of stars 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 Code for the computation of the structural and chemical evolution of stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Code for the computation of the structural and chemical evolution of stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-875031