dc.contributor.author |
Chakradhari, N. K |
|
dc.contributor.author |
Sahu, D. K |
|
dc.contributor.author |
Anupama, G. C |
|
dc.contributor.author |
Prabhu, T. P |
|
dc.date.accessioned |
2020-11-17T14:42:17Z |
|
dc.date.available |
2020-11-17T14:42:17Z |
|
dc.date.issued |
2018-02 |
|
dc.identifier.citation |
Monthly Notices of the Royal Astronomical Society, Vol. 474, No. 2, pp. 2502-2513 |
en_US |
dc.identifier.issn |
1365-2966 |
|
dc.identifier.uri |
http://prints.iiap.res.in/handle/2248/7189 |
|
dc.description |
Restricted Access © Royal Astronomical Society https://doi.org/10.1093/mnras/stx2839 |
en_US |
dc.description.sponsorship |
We present optical photometric and spectroscopic data for supernova SN 2004ab, a highly
reddened normal Type Ia supernova. The total reddening is estimated as E(B − V) =
1.70 ± 0.05 mag. The intrinsic decline-rate parameter m15(B)true is 1.27 ± 0.05, and the
B-band absolute magnitude at maximum MB max is −19.31 ± 0.25 mag. The host galaxy NGC
5054 is found to exhibit anomalous extinction with a very low value of RV = 1.41 ± 0.06 in the
direction of SN 2004ab. The peak bolometric luminosity is derived as log Lmax bol = 43.10 ± 0.07
erg s−1. The photospheric velocity measured from the absorption minimum of the Si II λ6355
line shows a velocity gradient of ˙ v = 90 km s−1 d−1, indicating that SN 2004ab is a member
of the high velocity gradient (HVG) subgroup. The ratio of the strengths of the Si II λ5972 and
λ6355 absorption lines, R(Si II), is estimated as 0.37, while their pseudo-equivalent widths
suggest that SN 2004ab belongs to the broad line (BL) type subgroup. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Oxford University Press on behalf of the Royal Astronomical Society |
en_US |
dc.subject |
Techniques: photometric |
en_US |
dc.subject |
Techniques: spectroscopic |
en_US |
dc.subject |
Supernovae: general |
en_US |
dc.subject |
Supernovae: individual: SN 2004ab |
en_US |
dc.subject |
Galaxies: individual: NGC 5054 |
en_US |
dc.title |
Highly Reddened Type Ia Supernova SN 2004ab: Another Case of Anomalous Extinction |
en_US |
dc.type |
Article |
en_US |