Astronomy:SN 1961i

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SN 1961i

SN 1961i was a supernova that was discovered in June 1961 in the Messier 61 (NGC 4303) galaxy, by Milton L. Humason at the Palomar Observatory,[1] the brightest of 16 supernovae found at Palomar that year.[2] Although it was originally considered by Fritz Zwicky to be the prototype of a type III supernova, subsequent researchers have classified it as a type II supernova.[3][4]

References

  1. Bertaud, C. (June 1961), "Les supernovae dans la nébuleuse NGC 4303", L'Astronomie 75: 268, Bibcode1961LAstr..75..268B .
  2. Humason, M. L.; Kearns, C. E.; Gomes, Alercio M. (June 1962), "The 1961 Palomar Supernova Search", Publications of the Astronomical Society of the Pacific (University of Chicago Press) 74: 215, doi:10.1086/127790, Bibcode1962PASP...74..215H .
  3. Doggett, J. B.; Branch, D. (November 1985), "A comparative study of supernova light curves", Astronomical Journal 90: 2303–2311, doi:10.1086/113934, Bibcode1985AJ.....90.2303D .
  4. Spiro, S.; Pastorello, A.; Pumo, M. L.; Zampieri, L.; Turatto, M.; Smartt, S. J. et al. (April 2014), "Low luminosity Type II supernovae - II. Pointing towards moderate mass precursors", Monthly Notices of the Royal Astronomical Society 439: 2873–2892, doi:10.1093/mnras/stu156, Bibcode2014MNRAS.439.2873S, http://repositorio.uchile.cl/bitstream/2250/127033/1/Low-luminosity-Type-II-supernovae-II-Pointing-towards-moderate-mass-precursors.pdf .

External links