STRONG EVOLUTION OF X-RAY ABSORPTION IN THE TYPE IIn SUPERNOVA SN 2010jl

Chandra, Poonam ; Chevalier, Roger A. ; Irwin, Christopher M. ; Chugai, Nikolai ; Fransson, Claes ; Soderberg, Alicia M. (2012) STRONG EVOLUTION OF X-RAY ABSORPTION IN THE TYPE IIn SUPERNOVA SN 2010jl The Astrophysical Journal, 750 (1). L2. ISSN 2041-8205

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Official URL: http://doi.org/10.1088/2041-8205/750/1/L2

Related URL: http://dx.doi.org/10.1088/2041-8205/750/1/L2

Abstract

We report two epochs of Chandra-ACIS X-ray imaging spectroscopy of the nearby bright Type IIn supernova SN 2010jl, taken around two months and then a year after the explosion. The majority of the X-ray emission in both spectra is characterized by a high temperature (≳ 10 keV) and is likely to be from the forward shocked region resulting from circumstellar interaction. The absorption column density in the first spectrum is high (∼1024 cm−2), more than three orders of magnitude higher than the Galactic absorption column, and we attribute it to absorption by circumstellar matter. In the second epoch observation, the column density has decreased by a factor of three, as expected for shock propagation in the circumstellar medium. The unabsorbed 0.2–10 keV luminosity at both epochs is ∼7 × 1041 erg s−1. The 6.4 keV Fe line clearly present in the first spectrum is not detected in the second spectrum. The strength of the fluorescent line is roughly that expected for the column density of circumstellar gas, provided the Fe is not highly ionized. There is also evidence for an absorbed power-law component in both spectra, which we attribute to a background ultraluminous X-ray source.

Item Type:Article
Source:Copyright of this article belongs to IOP Publishing
Keywords:circumstellar matter; hydrodynamics; supernovae: general; supernovae: individual: SN 2010jl; X-rays: general; Astrophysics - High Energy Astrophysical Phenomena
ID Code:125828
Deposited On:17 Oct 2022 08:53
Last Modified:17 Oct 2022 08:53

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