The eclipsing binary system W CRU

Details The eclipsing binary system W CRU The eclipsing binary system W CRU

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.150..103m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 150, no. 1, Dec. 1988, p. 103-113.

Astronomy and Astrophysics

Astrophysics

4

Eclipsing Binary Stars, Stellar Spectrophotometry, Ubv Spectra, Light Curve, Mass Transfer, Stellar Evolution, Stellar Mass, Stellar Temperature

Scientific paper

Photoelectric UBV observations of W Cru were obtained between 1984 and
1985 using the 50-cm Edith Winstone Blackwell Cassegrain telescope. The
light curve presents a continuous 'Beta Lyrae'-like variation, along
with peculier irregularities of the order of 0.1 mag. The possibility of
fitting both high-mass and low-mass models to the data is considered.

Affiliated with

Also associated with

No associations

Rating

The eclipsing binary system W CRU 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 The eclipsing binary system W CRU, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The eclipsing binary system W CRU will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1752767