No X-rays from the very nearby type Ia SN 2014J: Constraints on its environment

R. Margutti, J. Parrent, A. Kamble, A. M. Soderberg, R. J. Foley, D. Milisavljevic, M. R. Drout, R. Kirshner

Research output: Contribution to journalArticlepeer-review

82 Scopus citations

Abstract

Deep X-ray observations of the post-explosion environment around the very nearby Type Ia SN 2014J (d L = 3.5 Mpc) reveal no X-ray emission down to a luminosity Lx < 7 × 1036 erg s-1 (0.3-10 keV) at δt 20 days after the explosion. We interpret this limit in the context of inverse Compton emission from upscattered optical photons by the supernova shock and constrain the pre-explosion mass-loss rate of the stellar progenitor system to be (for wind velocity vw = 100 km s-1). Alternatively, the SN shock might be expanding into a uniform medium with density n CSM < 3 cm -3. These results rule out single-degenerate (SD) systems with steady mass loss until the terminal explosion and constrain the fraction of transferred material lost at the outer Lagrangian point to be ≤1%. The allowed progenitors are (1) white dwarf-white dwarf progenitors, (2) SD systems with unstable hydrogen burning experiencing recurrent nova eruptions with recurrence time t < 300 yr, and (3) stars where the mass loss ceases before the explosion.

Original languageEnglish (US)
Article number52
JournalAstrophysical Journal
Volume790
Issue number1
DOIs
StatePublished - Jul 20 2014

Keywords

  • supernovae: individual (SN 2014J)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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