Published August 1987
| Version v1
Journal article
Search for X-rays from the region of the Aries-Perseus flasher
Creators
- 1. Toronto Univ., Richmond Hill
- 2. Leiden Rijksuniversiteit, Netherlands
- 3. Amsterdam Universiteit, Netherlands
- 4. MIT, Cambridge, MA
Description
The region containing the Perseus flasher was observed for 5.4 h with the Exosat observatory. Upper limits to a point source with a steady X-ray flux were 2 x 10 to the -12th erg/sq cm s and 6 x 10 to the 12th erg/sq cm s. Upper limits to X-ray flashes of about 1 s duration were 4 x 10 to the 9th erg/sq cm s and 7 x 10 to the -10th erg/sq cm s. In view of the growing number of negative optical observations, it appears that either the optical flashes do not have a celestial origin, or that the flasher has a transient character and turns off for extended periods of time. 8 references
Additional details
Publishing Information
- Journal Title
- Astron. J.
- Journal Volume
- 94
- Series
- Astron. J.
- Journal Page Range
- 429-430
- ISSN
- 0004-6256
- CODEN
- ANJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19025269
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC X-RAY SOURCES; DATA PROCESSING; FLUX DENSITY; LIMITING VALUES; POINT SOURCES; RADIATION FLUX; VISIBLE SPECTRA; X-RAY SPECTRA
- Descriptors DEC
- COSMIC RAY SOURCES; RADIATION SOURCES; SPECTRA