A probable 1970 hard X-ray outburst by 4U 0041+32.
Abstract
Balloon observations of a hard X-ray burst in 1970 most likely associated with the highly variable high-latitude X-ray source 4U 0041+32 are reported. The observation of X-ray flux at a density of about 0.06 photons/sq cm per sec from a previously unknown source at r.a. O h 45 min, dec 33 + or - 3 deg was made by a scintillation telescope on February 4, 1970. The spectrum was found to be very hard between 25 and 300 keV, with radiation in the form of a well-collimated beam causing the excess counting rate over a period of 30 min. Further observations on September 25, 1970 indicated the object had faded to an intensity below 0.01 photons/sq cm per sec. The power law spectrum obtained during the February burst is observed to differ from those of other hard transients and hard compact binary X-ray sources by the fact that it extends to 300 keV, its apparent lack of pulsation and its not being associated with an early-type giant or supergiant companion.
- Publication:
-
Nature
- Pub Date:
- March 1980
- DOI:
- Bibcode:
- 1980Natur.284..324L
- Keywords:
-
- Balloon Flight;
- Cosmic X Rays;
- X Ray Sources;
- Balloon-Borne Instruments;
- Early Stars;
- Giant Stars;
- Oso-7;
- Power Spectra;
- Astrophysics;
- BALLOON FLIGHT;
- COSMIC X RAYS;
- X RAY SOURCES;
- BALLOON-BORNE INSTRUMENTS;
- EARLY STARS;
- GIANT STARS;
- OSO-7;
- POWER SPECTRA