Assaf Horesh et al. 2012 ApJ 746 21 doi:10.1088/0004-637X/746/1/21
Assaf Horesh1, S. R. Kulkarni1, Derek B. Fox2, John Carpenter1, Mansi M. Kasliwal1,3, Eran O. Ofek1,4, Robert Quimby5, Avishay Gal-Yam4, S. Bradley Cenko6, A. G. de Bruyn7,8, Atish Kamble9, Ralph A. M. J. Wijers9, Alexander J. van der Horst10, Chryssa Kouveliotou11, Philipp Podsiadlowski12, Mark Sullivan12, Kate Maguire12, D. Andrew Howell13,14, Peter E. Nugent15, Neil Gehrels16, Nicholas M. Law17, Dovi Poznanski18, and Michael Shara19
Show affiliationsOn 2011 August 24 (UT) the Palomar Transient Factory (PTF) discovered PTF11kly (SN 2011fe), the youngest and most nearby Type Ia supernova (SN Ia) in decades. We followed this event up in the radio (centimeter and millimeter bands) and X-ray bands, starting about a day after the estimated explosion time. We present our analysis of the radio and X-ray observations, yielding the tightest constraints yet placed on the pre-explosion mass-loss rate from the progenitor system of this supernova. We find a robust limit of
from sensitive X-ray non-detections, as well as a similar limit from radio data, which depends, however, on assumptions about microphysical parameters. We discuss our results in the context of single-degenerate models for SNe Ia and find that our observations modestly disfavor symbiotic progenitor models involving a red giant donor, but cannot constrain systems accreting from main-sequence or sub-giant stars, including the popular supersoft channel. In view of the proximity of PTF11kly and the sensitivity of our prompt observations, we would have to wait for a long time (a decade or longer) in order to more meaningfully probe the circumstellar matter of SNe Ia.
radio continuum: general; supernovae: general; X-rays: general
Issue 1 (2012 February 10)
Received 2011 September 13, accepted for publication 2011 October 25
Published 2012 January 20
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