Optical observables in stars with non-stationary atmospheres

Details Optical observables in stars with non-stationary atmospheres Optical observables in stars with non-stationary atmospheres

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cpsp.book..199h&link_type=abstract

In NASA. Goddard Space Flight Center Current Probl. in Stellar Pulsation Instabilities p 199-236 (SEE N80-25229 15-90)

Statistics

Computation

Cepheid Variables, Light Curve, Nuclear Explosions, Stellar Atmospheres, Stellar Models, Absorptivity, Doppler Effect, Hydrodynamics, Photosphere, Radiative Transfer, Shock Waves

Scientific paper

Experience gained by use of Cepheid modeling codes to predict the dimensional and photometric behavior of nuclear fireballs is used as a means of validating various computational techniques used in the Cepheid codes. Predicted results from Cepheid models are compared with observations of the continuum and lines in an effort to demonstrate that the atmospheric phenomena in Cepheids are quite complex but that they can be quantitatively modeled.

Affiliated with

Also associated with

No associations

Rating

Optical observables in stars with non-stationary atmospheres 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 Optical observables in stars with non-stationary atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical observables in stars with non-stationary atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1359248