Period lengthening in the V444 Cygni system and the mass loss by the Wolf--Rayet component
Journal Article
·
· Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6150932
New photoelectric photometry confirms that the period of V444 Cyg is lengthening at a rate P = 0.202 +- 0.018 sec/yr, implying a rate M = -(1.02 +- 0.20) x 10/sup -5/M/sub O//yr of mass loss by the WN5 component.
- Research Organization:
- Shternberg Astronomical Institute, Moscow
- OSTI ID:
- 6150932
- Journal Information:
- Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 10:4; ISSN SALED
- Country of Publication:
- United States
- Language:
- English
Similar Records
Period variation in the V444 Cygni system and mass loss by the Wolf--Rayet star
The period of V444 Cygni and its rate of change
Nature of the Wolf-Rayet component of the binary system V444 Cygni
Journal Article
·
Sun Jul 01 00:00:00 EDT 1979
· Sov. Astron. Lett. (Engl. Transl.); (United States)
·
OSTI ID:5790711
The period of V444 Cygni and its rate of change
Journal Article
·
Sun Jul 01 00:00:00 EDT 1990
· Publications of the Astronomical Society of the Pacific; (USA)
·
OSTI ID:6592941
Nature of the Wolf-Rayet component of the binary system V444 Cygni
Journal Article
·
Fri Oct 31 23:00:00 EST 1975
· Sov. Astron. AJ (Engl. Transl.); (United States)
·
OSTI ID:7190150