High Speed Photometry of AM CVns with the UCT CCD

Details High Speed Photometry of AM CVns with the UCT CCD High Speed Photometry of AM CVns with the UCT CCD

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..120w&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

Binaries: Close, Novae, Cataclysmic Variables, Stars: Individual (Es Cet, 2003Aw), Techniques: Photometric

Scientific paper

Following our high speed photometric survey of faint cataclysmic variables, two CVs were recognised to be helium-transferring double degenerates; these are ES Cet (P[orb] = 620.21144 s) and 2003aw (P[sh] = 2041.5 s). We have now observed ES Cet photometrically for over two years in order to follow the evolution of the orbital period. We offer an alternative explanation for the nature of V407 Vul (which was classified as an ultra-compact together with RX J0806 and ES Cet); this will take V407 Vul out of the AM CVn classification.

Affiliated with

Also associated with

No associations

Rating

High Speed Photometry of AM CVns with the UCT CCD 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 High Speed Photometry of AM CVns with the UCT CCD, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Speed Photometry of AM CVns with the UCT CCD will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-771855