No eclipses in the double WD binary SDSS J125733.63+542850.5

Details No eclipses in the double WD binary SDSS J125733.63+542850.5 No eclipses in the double WD binary SDSS J125733.63+542850.5

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2778....1s&link_type=abstract

The Astronomer's Telegram, #2778

Astronomy and Astrophysics

Astronomy

Optical, Binaries, Variables

Scientific paper

We have carried out a search with the Faulkes Telescope North (FTN) for eclipses in the binary white dwarf (WD) system SDSS J125733.63+542850.5, resulting in a non-detection. SDSS J125733.63+542850.5 was identified by Marsh et al. (2010) and Kulkarni & van Kerkwijk (2010) as a binary system consisting of a low-mass He WD (the primary) and a high-mass CO WD (the secondary), with an orbital period of 4.56 hours.

Affiliated with

Also associated with

No associations

Rating

No eclipses in the double WD binary SDSS J125733.63+542850.5 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 No eclipses in the double WD binary SDSS J125733.63+542850.5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and No eclipses in the double WD binary SDSS J125733.63+542850.5 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-978746