Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..130..485s&link_type=abstract
Astronomy and Astrophysics Supplement, v.130, p.485-494
Astronomy and Astrophysics
Astrophysics
28
Stars: Cataclysmic Variables, Stars: Individual: Al Com, V544 Her, V660 Her, V516 Cyg, Dx And
Scientific paper
In this paper we report photometric observations of AL Com, V544 Her, V660 Her, V516 Cyg and DX And taken during the descending phase after an outburst. For four of these variables we calibrated comparison stars in the field of view. Our observations cover the period in which AL Com showed the larger optical outburst since 1974, and V660 Her showed the larger outburst ever reported in the literature (B =~ 14.3). The optical spectral distribution of DX And, AL Com and V660 Her shows that the model of the steady-state accretion disk does not provide a good representation of the optical continuum during the decline phase of a dwarf nova outburst.
Fiorucci Massimo
Spogli Corrado
Tosti Gino
No associations
LandOfFree
BVRI observations of dwarf novae in outburst. I. AL Comae Berenices, V544 Herculis, V660 Herculis, V516 Cygni and DX Andromedae 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 BVRI observations of dwarf novae in outburst. I. AL Comae Berenices, V544 Herculis, V660 Herculis, V516 Cygni and DX Andromedae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BVRI observations of dwarf novae in outburst. I. AL Comae Berenices, V544 Herculis, V660 Herculis, V516 Cygni and DX Andromedae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1330336