Published 1979
| Version v1
Book
Observation of super-soft x-ray by the satellite 'Hakucho'
Description
Observation of super-soft X-ray has been made for the purposes to watch X-ray sources, to measure the X-ray spectra and to observe the variation of the sources in course of time. A detector for the present observation is a thin window proportional counter, which was separated to two sections. In other words, two independent counters are combined together. These counters are gas-flow type counters. The energy range of observed X-ray is from 0.1 to 2 KeV. The observation started on Feb. 21, 1979. Analysis of the obtained data is in progress. A burst from the burster 1636-536 and the strong variable X-ray star GX 339-4 were detected. The increase of light of the nova type variable UGem was observed on March 23. (Kato, T.)
Additional details
Additional titles
- Original title (Japanese)
- Kagaku eisei shinpojiumu.
Publishing Information
- Publisher
- Tokyo Univ., Inst. of Space and Aeronautical Science.
- Imprint Place
- Tokyo
- Imprint Title
- Symposium on the scientific satellite, 1978
- Journal Page Range
- p. 169-179.
Conference
- Title
- Symposium on the scientific satellite.
- Dates
- 24 - 26 May 1979.
- Place
- Tokyo, Japan.
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 12593837
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANGULAR DISTRIBUTION; COSMIC RADIATION; COSMIC RAY DETECTION; COSMIC X-RAY SOURCES; FLOW COUNTERS; SATELLITES; SOFT X RADIATION; X-RAY DETECTION
- Descriptors DEC
- COSMIC RAY SOURCES; DISTRIBUTION; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; MEASURING INSTRUMENTS; RADIATION DETECTION; RADIATION DETECTORS; RADIATIONS; X RADIATION
Optional Information
- Notes
- Imprint:Kagaku eisei shinpojiumu.