On the spectrum of supernova 1972e in NGC 5253

Details On the spectrum of supernova 1972e in NGC 5253 On the spectrum of supernova 1972e in NGC 5253

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84.1837b&link_type=abstract

Astronomical Journal, vol. 84, Dec. 1979, p. 1837-1839.

Astronomy and Astrophysics

Astronomy

13

Astronomical Spectroscopy, Electrophotometry, Stellar Spectra, Supernovae, Emission Spectra, Line Spectra, Wavelengths

Scientific paper

Photoelectric scans of the spectrum of SN 1972e are presented. The observations were obtained at the McDonald Observatory between 15 and 50 days after maximum light with a spectral resolution ranging from 4 to 20 A. Line identifications (Ca II, Fe II, Si II, and possibly He I) are discussed briefly. It is suggested that the emission feature identified by Kirshner and Oke (1975) as H alpha may have been produced by Fe II.

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