A comment on the very high (>= 1015 eV) gamma ray from Cyg X-3 based on the data of Akeno Observatory
Description
Gamma ray data from Cyg X-3 observed at Akeno Observatory for more than three years since early 1981 were analyzed and main results are briefly presented here. Periodic changes were compared with those of X-ray (period 4.8 hours) observed and reported by Parsignault et al. or by Van der Klis and Bonnet-Bidault. The coincidence of periods of both gamma ray and X ray was tested by the method of harmonic analysis and was proved not to be an accidental coincidence. A statistically meaningful correlation with fluctuation of X-ray from Cyg X-3 is observed only in the direction of Cyg X-3. This suggests existence of some physical meaning. Other analyses including gamma ray absolute flux, shower age, and lateral distribution of muon are now underway. (Aoki, K.)
Additional details
Publishing Information
- Journal Title
- Uchusen Kenkyu
- Journal Volume
- 28
- Journal Issue
- 2
- Series
- Uchusen Kenkyu.
- Journal Page Range
- 157-161
- ISSN
- 0386-6971
- CODEN
- UCKEA
Conference
- Title
- Study meeting on cosmic ray composition in high energy region.
- Dates
- 1-2 Nov 1984.
- Place
- Tanashi, Tokyo (Japan).
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 17071079
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC GAMMA SOURCES; DAILY VARIATIONS; FREQUENCY ANALYSIS; GAMMA RADIATION; PEV RANGE; PRIMARY COSMIC RADIATION
- Descriptors DEC
- COSMIC RADIATION; COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; ENERGY RANGE; IONIZING RADIATIONS; RADIATIONS; VARIATIONS