Published December 1988
| Version v1
Journal article
High-speed photometry of dwarf nova SS Cygni
Creators
- 1. Moskovskij Gosudarstvennyj Univ., Moscow (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''
Description
Quasi-periodic oscillations with full amplitude of 1.5% have been found for SS Cyg in the decline from the 1982 September outburst (maximum light 1982 September 16). These oscillations were observed in the V band and U band light curves on the night of September 20, but no pulsations were observed on the previous night September 19 in the limits of accuracy. Possibly, the new third group of oscillations in SS Cyg have been detected
Additional details
Additional titles
- Original title (Russian)
- Высокоскоростная фотометрия карликовой новой SS Лебедя
Publishing Information
- Journal Title
- Astrofizika
- Journal Volume
- 29
- Journal Issue
- 3
- Series
- Astrofizika.
- Journal Page Range
- 433-439
- ISSN
- 0571-7132
- CODEN
- ASTKB
INIS
- Country of Publication
- Armenia
- Country of Input or Organization
- USSR
- INIS RN
- 21008950
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- BINARY STARS; BRIGHTNESS; DWARF STARS; EXPERIMENTAL DATA; NOVAE; OSCILLATIONS; PHOTOMETRY; STELLAR RADIATION; TIME DEPENDENCE
- Descriptors DEC
- DATA; ERUPTIVE VARIABLE STARS; INFORMATION; NUMERICAL DATA; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STARS; VARIABLE STARS