Long-term decrease and cyclic variation in the orbital period of the eclipsing dwarf NOVA V2051 OPH
Journal Article
·
· Astrophysical Journal, Supplement Series
- Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650011 Kunming (China)
V2051 Oph is a deeply eclipsing dwarf nova with an orbital period below the period gap of cataclysmic variables (CVs). It has been photometrically monitored since 2008 June and 24 mid-eclipse times of the white dwarf have been obtained. The changes in the orbital period are investigated using all of the available mid-eclipse times.
- OSTI ID:
- 22879409
- Journal Information:
- Astrophysical Journal, Supplement Series, Journal Name: Astrophysical Journal, Supplement Series Journal Issue: 1 Vol. 221; ISSN 0067-0049; ISSN APJSA2
- Country of Publication:
- United States
- Language:
- English
Similar Records
ORBITAL PERIODS FOR THREE RECURRENT NOVAE
Periodicities and disks in dwarf novae
SW UMa and V426 Oph: EXOSAT surprises
Journal Article
·
Wed May 20 00:00:00 EDT 2009
· Astrophysical Journal
·
OSTI ID:21300567
Periodicities and disks in dwarf novae
Journal Article
·
Sun Dec 09 23:00:00 EST 1973
· Nature (London) Phys. Sci., v. 246, no. 154, pp. 84-87
·
OSTI ID:4348989
SW UMa and V426 Oph: EXOSAT surprises
Book
·
Thu Dec 31 23:00:00 EST 1987
·
OSTI ID:6740324