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

ABSTRACT 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 20...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2020-09, Vol.497 (3), p.3770-3789
Hauptverfasser: Gangopadhyay, Anjasha, Misra, Kuntal, Sahu, D K, Wang, Shan-Qin, Kumar, Brajesh, Li, Long, Anupama, G C, Dastidar, Raya, Elias-Rosa, N, Kumar, Brijesh, Singh, Mridweeka, Pandey, S B, Sanwal, Pankaj, Singh, Avinash, Srivastav, S, Tartaglia, L, Tomasella, L
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Sprache:eng
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Zusammenfassung:ABSTRACT 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 × 1014 and 35.3 × 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⊙.
ISSN:0035-8711
1365-2966
1365-2966
DOI:10.1093/mnras/staa1821