Upper limits on Co-57 abundance in SN1987A according to the KVANT data

Details Upper limits on Co-57 abundance in SN1987A according to the KVANT data Upper limits on Co-57 abundance in SN1987A according to the KVANT data

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..171s&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 171-172 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

Abundance, Cobalt Isotopes, Stellar Composition, Supernova 1987A, Mir Space Station, Pulsars, Stellar Spectra, X Ray Spectra

Scientific paper

Seven hard X-ray spectra of SN1987A obtained at different times by instruments onboard Kvant module are presented. During June observations the flux from the supernova was not detected. Only three sigma limits are presented. The 50-millisecond pulsar PSR 0540-693 and LMC X-1 were also in the field of view of HEXE instrument during the June observations.

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