Photometric elements of the eclipsing binary OX CAS

Details Photometric elements of the eclipsing binary OX CAS Photometric elements of the eclipsing binary OX CAS

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....82..386m&link_type=abstract

Astronomy and Astrophysics, vol. 82, no. 3, Feb. 1980, p. 386, 387. Research supported by the Consiglio Nazionale delle Ricerch

Astronomy and Astrophysics

Astrophysics

3

B Stars, Eclipsing Binary Stars, Stellar Spectrophotometry, Ubv Spectra, Light Curve, Stellar Luminosity, Stellar Temperature

Scientific paper

UBV lightcurves - as yet unsolved - of the B spectral type eclipsing binary OX Cas (Frazier and Hall, 1975) have been analyzed by means of Wood's (1972) model. OX Cas turned to be composed of two detached components having very nearly equal temperatures, but appreciably different sizes and luminosities. The hotter star is larger and brighter than its cooler companion.

Affiliated with

Also associated with

No associations

Rating

Photometric elements of the eclipsing binary OX CAS 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 Photometric elements of the eclipsing binary OX CAS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric elements of the eclipsing binary OX CAS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620253