Space and ground-based spectrophotometric observations of a group of stars of the classes F, G, and K

Details Space and ground-based spectrophotometric observations of a group of stars of the classes F, G, and K Space and ground-based spectrophotometric observations of a group of stars of the classes F, G, and K

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981afz....17..495e&link_type=abstract

(Astrofizika, vol. 17, July-Sept. 1981, p. 495-508.) Astrophysics, vol. 17, no. 3, Jan. 1982, p. 277-285. Translation.

Astronomy and Astrophysics

Astronomy

1

F Stars, G Stars, Giant Stars, Ground Truth, K Stars, Spectral Energy Distribution, Stellar Spectra, Stellar Spectrophotometry, Supergiant Stars, Atmospheric Models, Binary Stars, Stellar Atmospheres, Stellar Luminosity, Ultraviolet Astronomy

Scientific paper

The paper presents spectrophotometric measurements of 22 stars of the intermediate spectral classes F, G, and K, in the region of the sky around Capella in the wavelength range from 2400 to 4800 A. Ultraviolet observations and combined spectra are used to find the luminosity classes of the components of binaries. Concrete examples are used to show that the combined space and ground-based method of observations of star spectra can be effective in discovering an invisible high-temperature component of low luminosity in a binary system, and in establishing the presence of a giant or supergiant of intermediate or late class as one of the components of unresolved binaries.

Affiliated with

Also associated with

No associations

Rating

Space and ground-based spectrophotometric observations of a group of stars of the classes F, G, and K 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 Space and ground-based spectrophotometric observations of a group of stars of the classes F, G, and K, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Space and ground-based spectrophotometric observations of a group of stars of the classes F, G, and K will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1687488