Photometry of the Newly-Discovered SU UMa Star in Taurus

Details Photometry of the Newly-Discovered SU UMa Star in Taurus Photometry of the Newly-Discovered SU UMa Star in Taurus

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..938....1s&link_type=abstract

The Astronomer's Telegram, #938

Astronomy and Astrophysics

Astronomy

1

Optical, Cataclysmic Variables

Scientific paper

We report the results of time-resolved CCD photometry obtained with the Mount Laguna Observatory 1-m reflector of the recently-discovered variable star in Taurus (CBET #701). A total of ~20 hours of V-band photometry over six nights (2006 Oct 28 - 30; 2006 Nov 01 - 03) has enabled us to confirm its tentative identification as a previously unknown SU UMa dwarf nova, and to establish a revised superhump period of 0.05338(1) days (76.87 min).

Affiliated with

Also associated with

No associations

Rating

Photometry of the Newly-Discovered SU UMa Star in Taurus 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 Photometry of the Newly-Discovered SU UMa Star in Taurus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometry of the Newly-Discovered SU UMa Star in Taurus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1311600