Spectral classes of the cold components of U GEM type stars

Details Spectral classes of the cold components of U GEM type stars Spectral classes of the cold components of U GEM type stars

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....21..289t&link_type=abstract

(Astrofizika, vol. 21, Sept.-Oct. 1984, p. 289-294) Astrophysics (ISSN 0571-7132), vol. 20, no. 5, March 1985, p. 507-510. Trans

Astronomy and Astrophysics

Astrophysics

3

Companion Stars, Dwarf Novae, Stellar Luminosity, Stellar Orbits, Stellar Spectra, Main Sequence Stars, Stellar Flares

Scientific paper

A relationship has been found between the orbital period of U Gem binary systems and the spectral class of their cold components. The existence of this relation may make it possible to determine the spectral class of the cold components of such stars that are difficult to observe. In addition, it follows from the orbital-period-mass and orbital-period-spectral-class relations of the cold components that they are on the main sequence. This makes it possible to estimate the luminosities of the cold components from the revolution period.

Affiliated with

Also associated with

No associations

Rating

Spectral classes of the cold components of U GEM type 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 Spectral classes of the cold components of U GEM type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral classes of the cold components of U GEM type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1389852