Published August 1987 | Version v1
Journal article

Search for X-rays from the region of the Aries-Perseus flasher

  • 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