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2021ApJ...909..100S - Astrophys. J., 909, 100-100 (2021/March-2)

The fast-evolving Type Ib supernova SN 2015dj in NGC 7371.

SINGH M., MISRA K., VALENTI S., HOSSEINZADEH G., PASTORELLO A., SRIVASTAV S., GANGOPADHYAY A., DASTIDAR R., TOMASELLA L., ARCAVI I., BENETTI S., CALLIS E., CAPPELLARO E., ELIAS-ROSA N., HOWELL D.A., KIM S.C., McCULLY C., TARTAGLIA L., TERRERAN G. and TURATTO M.

Abstract (from CDS):

We present the detailed optical evolution of a Type Ib SN 2015dj in NGC 7371, using data spanning up to ∼170 days after discovery. SN 2015dj shares similarity in light-curve shape with SN 2007gr and peaks at MV = -17.37 ± 0.02 mag. Analytical modeling of the quasi bolometric light curve yields 0.06 ± 0.01 M of 56Ni, ejecta mass Mej=1.4–0.5+1.3M, and kinetic energy Ek=0.7–0.3+0.6×1051 erg. The spectral features show a fast evolution and resemble those of spherically symmetric ejecta. The analysis of nebular phase spectral lines indicates a progenitor mass between 13-20 M, suggesting a binary scenario.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Type Ib supernovae - Core-collapse supernovae

Simbad objects: 17

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