Algol-type binaries

Details Algol-type binaries Algol-type binaries

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988lastr.102..528h&link_type=abstract

L'Astronomie (ISSN 0004-6302), vol. 102, Dec. 1988, p. 528-532. In French.

Other

Eclipsing Binary Stars, Light Curve, Stellar Spectra, Cool Stars, Stellar Evolution, Stellar Luminosity, Stellar Temperature, Variable Stars

Scientific paper

Various scenarios for the ejection of matter by the primary component of Algol binaries are possible, depending on the masses of the two component and on their distance from each other. Algol-type binaries are characterized by irregularly variable periods. IUE observations reveal that certain Algols have elevated Al III, Fe III, Si IV, C IV, and N V ionization levels.

Affiliated with

Also associated with

No associations

Rating

Algol-type binaries 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 Algol-type binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Algol-type binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1758891