dc.contributor.author |
Singh, A |
|
dc.contributor.author |
Srivastav, S |
|
dc.contributor.author |
Brajesh Kumar |
|
dc.contributor.author |
Anupama, G. C |
|
dc.contributor.author |
Sahu, D. K |
|
dc.date.accessioned |
2020-11-11T07:45:13Z |
|
dc.date.available |
2020-11-11T07:45:13Z |
|
dc.date.issued |
2018-10 |
|
dc.identifier.citation |
Monthly Notices of the Royal Astronomical Society, Vol. 480, No. 2, pp. 2475-2500 |
en_US |
dc.identifier.issn |
1365-2966 |
|
dc.identifier.uri |
http://prints.iiap.res.in/handle/2248/6915 |
|
dc.description |
Restricted Access © Royal Astronomical Society; https://doi.org/10.1093/mnras/sty1957 |
en_US |
dc.description.abstract |
Optical broadband (UBVRI) photometric and low-resolution spectroscopic observations of the Type II-P supernova (SN) ASASSN-14dq are presented. ASASSN-14dq exploded in a low-luminosity/metallicity host galaxy UGC 11860, the signatures of which are present as weak iron lines in the photospheric phase spectra. The SN has a plateau duration of ∼90 d, with a plateau decline rate of 1.38 mag (100d)−1 in the V-band, which is higher than most Type II-P SNe. ASASSN-14dq is a luminous Type II-P SN with a peak V-band absolute magnitude of –17.7 ±0.2 mag. The light curve of ASASSN-14dq indicates it to be a fast-declining Type II-P SN, making it a transitional event between Type II-P and II-L SNe. The empirical relation linking the steepness parameter and 56Ni mass for Type II SNe was rebuilt with the help of well-sampled light curves from the literature. The estimated 56Ni mass of ∼0.029 M⊙ for ASASSN-14dq is slightly lower for a luminous Type II-P SN. Using analytical light curve modelling, a progenitor radius of ∼3.6×1013 cm, an ejecta mass of ∼10 M⊙, and total energy of ∼1.8×1051 erg were estimated for this event. The photospheric velocity evolution of ASASSN-14dq resembles that of a Type II-P SN, but the Balmer features (H α and H β) show relatively slow velocity evolution. The high-velocity H α feature in the plateau phase, the asymmetric H α emission line profile in the nebular phase, and the inferred outburst parameters indicate an interaction of the SN ejecta with the circumstellar material. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Oxford University Press on behalf of the Royal Astronomical Society |
en_US |
dc.subject |
Supernovae: general |
en_US |
dc.subject |
Supernovae: individual: ASASSN-14dq |
en_US |
dc.subject |
Galaxies: individual: UGC 11860 |
en_US |
dc.title |
ASASSN-14dq: A fast-declining type II-P Supernova in a low-luminosity host galaxy |
en_US |
dc.type |
Article |
en_US |