Spectrophotometry of the RS CVn stars. I - The F, G, and K standards

Details Spectrophotometry of the RS CVn stars. I - The F, G, and K standards Spectrophotometry of the RS CVn stars. I - The F, G, and K standards

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..665a&link_type=abstract

Astronomical Journal, vol. 87, Apr. 1982, p. 665-669.

Astronomy and Astrophysics

Astronomy

6

Eclipsing Binary Stars, F Stars, G Stars, Giant Stars, K Stars, Spectral Energy Distribution, Stellar Spectrophotometry, Continuous Spectra, Near Infrared Radiation, Stellar Evolution, Stellar Temperature, Subgiant Stars, Visible Spectrum

Scientific paper

The Varian LSE tube used to observe RS Canum Venaticorum-type binary stars is discussed. The instrument allows simultaneous observation in both the photographic and the near-infrared regions. The energy distributions of 14 standard F, G, and K stars are presented, and the morphology of the energy distribution as a function of spectral type is shown. Bandpasses of specific interest are indicated. The b-y colors are synthesized and effective temperatures are found. The model atmospheres can be arranged in a simple one-dimensional grid analogous to the original HD system for stars less luminous than giants.

Affiliated with

Also associated with

No associations

Rating

Spectrophotometry of the RS CVn stars. I - The F, G, and K standards 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 Spectrophotometry of the RS CVn stars. I - The F, G, and K standards, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrophotometry of the RS CVn stars. I - The F, G, and K standards will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-840249