SN 2004A: Another Type II-P Supernova with a Red Supergiant Progenitor
Abstract
We present a monitoring study of SN 2004A and probable discovery of a progenitor star in pre-explosion HST images. The photometric and spectroscopic monitoring of SN 2004A show that it was a normal Type II-P which was discovered in NGC 6207 about two weeks after explosion. We compare SN 2004A to the similar Type II-P SN 1999em and estimate an explosion epoch of 2004 January 6. We also calculate three new distances to NGC 6207 of 21.0 +/-4.3, 21.4 +/-3.5 and 25.1 +/-1.7Mpc. The former was calculated using the Standard Candle Method (SCM) for SNe II-P, and the latter two from the Brightest Supergiants Method (BSM). We combine these three distances with existing kinematic distances, to derive a mean value of 20.3 +/-3.4Mpc. Using this distance we estimate that the ejected nickel mass in the explosion is 0.046(+0.031,-0.017) Msolar. The progenitor of SN 2004A is identified in pre-explosion WFPC2 F814W images with a magnitude of mF814W = 24.3 +/-0.3, but is below the detection limit of the F606W images. We show that this was likely a red supergiant (RSG) with a mass of 9(+3,-2) Msolar. The object is detected at 4.7 sigma above the background noise. Even if this detection is spurious, the 5 sigma upper limit would give a robust upper mass limit of 12 Msolar for a RSG progenitor. These initial masses are very similar to those of two previously identified RSG progenitors of the Type II-P SNe 2004gd 8(+4,-2) Msolar and 2005cs 9(+3,-2) Msolar).
Keywords
Cite
@article{arxiv.astro-ph/0603670,
title = {SN 2004A: Another Type II-P Supernova with a Red Supergiant Progenitor},
author = {M. A. Hendry and S. J. Smartt and R. M. Crockett and J. R. Maund and A. Gal-Yam and D. -S. Moon and S. B. Cenko and D. W. Fox and R. P. Kudritzki and C. R. Benn and R. Østensen},
journal= {arXiv preprint arXiv:astro-ph/0603670},
year = {2016}
}
Comments
Accepted for publication in MNRAS; 20 pages, 14 figures; corrected scale on Fig. 1