Discovery of an unusual hard X-ray source in the region of supernova 1987A

We have discovered a new hard X-ray source near supernova 1987 A, in the Large Magellanic Cloud, from the X-ray astronomy satellite Ginga. The present error box of 0.2 ° × 0.3 ° includes the supernova. The energy spectrum is very hard above 10 keV and unusual for any of the known classes of X-ray so...

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Veröffentlicht in:Nature (London) 1987-11, Vol.330 (6145), p.230-231
Hauptverfasser: Dotani, T, Hayashida, K, Inoue, H, Itoh, M, Koyama, K, Makino, F, Mitsuda, K, Murakami, T, Oda, M, Ogawara, Y, Takano, S, Tanaka, Y, Yoshida, A, Makishima, K, Ohashi, T, Kawai, N, Matsuoka, M, Hoshi, R, Hayakawa, S, Kii, T, Kunieda, H, Nagase, F, Tawara, Y, Hatsukade, I, Kitamoto, S, Miyamoto, S, Tsunemi, H, Yamashita, K, Nakagawa, M, Yamauchi, M, Turner, M. J. L, Pounds, K. A, Thomas, H. D, Stewart, G. C, Cruise, A. M, Patchett, B. E, Reading, D. H
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Sprache:eng
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Zusammenfassung:We have discovered a new hard X-ray source near supernova 1987 A, in the Large Magellanic Cloud, from the X-ray astronomy satellite Ginga. The present error box of 0.2 ° × 0.3 ° includes the supernova. The energy spectrum is very hard above 10 keV and unusual for any of the known classes of X-ray source. The flux in the range 10–30 keV as of 2–3 September is ˜5×10 –11 ergcm –2 s –1 . The source intensity increased steadily throughout July, August and early September, but an observation in late September revealed no further increase. The positional agreement, a steady brightening and an unusual hard spectrum support the identification of the source as SN1987A.
ISSN:0028-0836
1476-4687
DOI:10.1038/330230a0