CCD photometry of variable stars in the Magellanic Clouds. III - The eclipsing binary HV 12484

Details CCD photometry of variable stars in the Magellanic Clouds. III - The eclipsing binary HV 12484 CCD photometry of variable stars in the Magellanic Clouds. III - The eclipsing binary HV 12484

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.260..777t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 260, no. 4, p. 777-781.

Astronomy and Astrophysics

Astronomy

10

Astronomical Photometry, Charge Coupled Devices, Eclipsing Binary Stars, Magellanic Clouds, Variable Stars, Early Stars, Ephemeris Time, Light Curve

Scientific paper

B, V, and I photometry is presented for the eclipsing binary HV 12484 located in the Large Magellanic Cloud. The system is detached and seen close to edge-on. Any orbital eccentricity is slight. A new ephemeris is derived. Analysis with Etzel's EBOP code shows that the component stars can differ by no more than about 10 percent in radius. The system could plausibly comprise stars broadly similar to B2 IV galactic stars separated by about three times their radius.

Affiliated with

Also associated with

No associations

Rating

CCD photometry of variable stars in the Magellanic Clouds. III - The eclipsing binary HV 12484 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 CCD photometry of variable stars in the Magellanic Clouds. III - The eclipsing binary HV 12484, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD photometry of variable stars in the Magellanic Clouds. III - The eclipsing binary HV 12484 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1275959