Infrared light curves of Type I supernovae. II - Late stages

Details Infrared light curves of Type I supernovae. II - Late stages Infrared light curves of Type I supernovae. II - Late stages

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...268..718e&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 268, May 15, 1983, p. 718-720.

Astronomy and Astrophysics

Astrophysics

8

Infrared Spectra, Light Curve, Stellar Color, Supernovae, Galactic Nuclei, Stellar Magnitude, Stellar Spectrophotometry

Scientific paper

Infrared light curves of three Type I supernovae obtained by Elias et al. (1981) are extended to approximately one year after maximum light. The light curves and colors show no evidence for the development of an infrared excess. The very red J-H color observed roughly 100 days after maximum becomes bluer, probably indicating decreased absorption at 1.2 micron.

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