SIMBAD references

2020MNRAS.497.3770G - Mon. Not. R. Astron. Soc., 497, 3770-3789 (2020/September-3)

Optical studies of two stripped-envelope supernovae - SN 2015ap (Type Ib) and SN 2016P (Type Ic).

GANGOPADHYAY A., MISRA K., SAHU D.K., WANG S.-Q., KUMAR B., LI L., ANUPAMA G.C., DASTIDAR R., ELIAS-ROSA N., KUMAR B., SINGH M., PANDEY S.B., SANWAL P., SINGH A., SRIVASTAV S., TARTAGLIA L. and TOMASELLA L.

Abstract (from CDS):

We present the photometric and spectroscopic studies of a Type Ib SN 2015ap and a Type Ic SN 2016P. SN 2015ap is one of the bright (MV = -18.04 mag) Type Ib while SN 2016P lies at an average value among the Type Ic SNe (MV = -17.53 mag). Bolometric light-curve modelling of SNe 2015ap and 2016P indicates that both the SNe are powered by 56Ni + magnetar model with 56Ni masses of 0.01 and 0.002 M☉, ejecta masses of 3.75 and 4.66 M☉, spin period P0 of 25.8 and 36.5 ms, and magnetic field Bp of 28.39 x 1014 and 35.3 x 1014 G, respectively. The early spectra of SN 2015ap show prominent lines of He with a 'W' feature due to Fe complexes while other lines of Mg II, Na I, and Si II are present in both SNe 2015ap and 2016P. Nebular phase [O I] profile indicates an asymmetric profile in SN 2015ap. The [O I]/[Ca II] ratio and nebular spectral modelling of SN 2015ap hint towards a progenitor mass between 12 and 20 M☉.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): techniques: photometric - techniques: spectroscopic - supernovae: general - supernovae: individual: (SNe 2015ap, 2016P) - galaxies: individual: (IC 1776, NGC 5374) - transients: supernovae

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 54

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