Hard X-rays from supernova 1987A
Autor: | D. Stepanov, A. Prudkoglyad, Joachim Trümper, R. A. Sunyaev, V. Loznikov, A. Mclioransky, Wolfgang Voges, S. Unin, Wolfgang Pietsch, M. Bezler, Rüdiger Staubert, Eckhard Kendziorra, A. V. Kuznetsov, S. A. Grebenev, Claus Reppin, V. Efremov, A. S. Kaniovsky, Jakob Englhauser |
---|---|
Rok vydání: | 1990 |
Předmět: |
Physics
Atmospheric Science X-ray astronomy Astrophysics::High Energy Astrophysical Phenomena Aerospace Engineering Astronomy Astronomy and Astrophysics Spectral bands Astrophysics Light curve Astronomical spectroscopy Supernova Geophysics Pulsar Space and Planetary Science Observatory General Earth and Planetary Sciences Large Magellanic Cloud Astrophysics::Galaxy Astrophysics |
Zdroj: | Advances in Space Research. 10:47-53 |
ISSN: | 0273-1177 |
DOI: | 10.1016/0273-1177(90)90117-i |
Popis: | On 10 August 1987, the HEXE instrument on the MIR-KVANT observatory ROENTGEN detected hard X-ray emission from the region of Supernova 1987A in the Large Magellanic Cloud in the 20–100 keV spectral band at a 10 standard deviation level. From then on SN 1987A became the main observation target. During the August observations of SN 1987A the PULSAR X-1 instrument detected a significant X-ray flux from the region of the Supernova in the 50–300 keV energy band. The HEXE data allowed an accurate localization of the hard X-ray source, and the calculated position coincides well with that of SN 1987A. Other well-known X-ray sources were outside the 3 σ-error box. |
Databáze: | OpenAIRE |
Externí odkaz: |