A Grid of Model Atmospheres for Cool Stars

Details A Grid of Model Atmospheres for Cool Stars A Grid of Model Atmospheres for Cool Stars

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..288..331g&link_type=abstract

Stellar Atmosphere Modeling, ASP Conference Proceedings, Vol. 288. Abstracts from a conference held 8-12 April 2002 in Tuebingen

Astronomy and Astrophysics

Astronomy

108

Scientific paper

An extensive grid of spherically symmetric model atmospheres of stars with
1. 2500 K ≤ Teff ≤ 8000 K, 2. -1.0 ≤ log g (= log GM/R2) ≤ 5.0 (cgs units), 3. different combinations of M and R, 4. -5 ≤ [A/H] ≤ 1, and 5. a number of CNO abundance combinations
is being constructed with an updated version of the MARCS program.
Special efforts are made to reach accuracy and completeness in opacity data. Opacity sampling is used with 10,000 and (for a minority of models) 90,000 wavelength points. Synthetic spectra are also provided.
We shall show how these classical models may be used to illustrate important physical properties of cool star atmospheres.

Affiliated with

Also associated with

No associations

Rating

A Grid of Model Atmospheres for Cool 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 A Grid of Model Atmospheres for Cool Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Grid of Model Atmospheres for Cool Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1526076