A spectrum synthesis program for binary stars

Details A spectrum synthesis program for binary stars A spectrum synthesis program for binary stars

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...434..738l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 434, no. 2, p. 738-746

Computer Science

Numerical Analysis

15

Astronomical Spectroscopy, Computer Programs, Computerized Simulation, Eclipsing Binary Stars, Spectra, Stellar Models, Distortion, Doppler Effect, Numerical Analysis, Radial Velocity, Stellar Rotation, Stellar Temperature

Scientific paper

A new program produces synthetic spectra of binary stars at arbitrary values of orbital longitude, including longitudes of partial or complete eclipse. The stellar components may be distorted, either tidally or rotationally, or both. Either or both components may be rotating nonsynchronously. We illustrate the program performance with two cases: EE Peg, an eclipsing binary with small distortion, and SX Aur, an eclipsing binary that is close to contact.

Affiliated with

Also associated with

No associations

Rating

A spectrum synthesis program for binary 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 spectrum synthesis program for binary stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A spectrum synthesis program for binary stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1070528