Astronomy:SN 2004dj

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Short description: July 2004 supernova event in the constellation Camelopardalis
SN 2004dj
Spectral classII-P
Date31 July 2004 18:15 UTC
ConstellationCamelopardalis
Right ascension07h 37m 17.044s
Declination+65° 35 57.84″
EpochJ2000.0
Galactic coordinates?
Distanceabout 11,000,000 light-years [1]
RemnantNebula
HostNGC 2403
ProgenitorUnknown star in compact cluster Sandage 96
Progenitor typeSupergiant
Colour (B-V)Unknown
Notable featuresLight Curves
Peak apparent magnitude+11.2

SN 2004dj was the brightest supernova since SN 1987A at the time of its discovery.[1]

A light curve for SN 2004dj, plotted from AAVSO data[2]

This Type II-P supernova was discovered by Japanese astronomer Kōichi Itagaki on 31 July 2004. At the time of its discovery, its apparent brightness was 11.2 visual magnitude; the discovery occurred after the supernova had reached its peak magnitude.[3][4] The supernova's progenitor is a star in a young, compact star cluster in the galaxy NGC 2403, in Camelopardalis. The cluster had been cataloged as the 96th object in a list of luminous stars and clusters by Allan Sandage in 1984; the progenitor is therefore commonly referred to as Sandage 96. This cluster is easily visible in a Kitt Peak National Observatory image and appears starlike.

References

  1. Bishop, David. "Bright Supernovae - 2004". https://www.rochesterastronomy.org/sn2004/index.html. 
  2. "Download Data". AAVSO. https://www.aavso.org/data-download. 
  3. Nakano, S.; Itagaki, K.; Bouma, R. J.; Lehky, M.; Hornoch, K. (2004-08-01). "Supernova 2004dj in NGC 2403". International Astronomical Union Circular (8377): 1. ISSN 0081-0304. Bibcode2004IAUC.8377....1N. https://ui.adsabs.harvard.edu/abs/2004IAUC.8377....1N. 
  4. A. J., Nayana; Chandra, Poonam; K. Ray, Alak (2018-08-20). "Long-term Behavior of a Type IIP Supernova SN 2004dj in the Radio Bands". The Astrophysical Journal 863 (2): 163. doi:10.3847/1538-4357/aad17a. ISSN 1538-4357. Bibcode2018ApJ...863..163N.