Photometric and spectral observations of the Supernova 1987A

Details Photometric and spectral observations of the Supernova 1987A Photometric and spectral observations of the Supernova 1987A

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...89z&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, May-June 1988, p. 89-91. In Russian.

Astronomy and Astrophysics

Astronomy

Stellar Spectrophotometry, Supernova 1987A, Astronomical Observatories, Bolivia, H Lines, Polarimetry, Ubv Spectra

Scientific paper

Photometric (UBVR) and spectral observations of Supernova 1987A in the LMC obtained at the Bolivian-Soviet observatory near Tarija, Bolivia during April-August, 1987 are presented. A spectrophotopolarimeter mounted at the Cassegrain (F = 7.5 m) focus of the Zeiss 60-cm reflector was used. It was found that, for Supernova 1987A, the UV part of the spectrum was weakened during March 7-July 9, 1987. There was a simultaneous increase in brightness, and hydrogen emission lines characteristic of type II supernovae were present.

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