A hard extended X-ray source in the IC 443 supernova remnant resolved by Chandra

A fast ejecta fragment or a new pulsar wind nebula?

A. M. Bykov, F. Bocchino, George Pavlov

Research output: Contribution to journalArticle

14 Citations (Scopus)

Abstract

A Chandra observation of the isolated hard X-ray source XMMU J061804.3+222732, located in the region of the apparent interaction of the supernova remnant IC 443 with a molecular cloud, resolved the complex structure of the source in a few bright clumps embedded in an extended emission of ∼30″ in size. The X-ray spectra of the clumps and the extended emission are dominated by a hard power-law component with a photon index of 1.2-1.4. In addition, we see some indications of an optically thin thermal plasma of an ∼0.3 keV temperature. The observed X-ray morphology and spectra are consistent with those expected for an isolated supernova ejecta fragment interacting with a dense ambient medium. A possible alternative interpretation is a pulsar wind nebula associated with either IC 443 or another supernova remnant, G189.6+3.3.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume624
Issue number1 II
DOIs
StatePublished - May 1 2005

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supernova remnants
ejecta
nebulae
pulsars
fragments
clumps
x rays
thermal plasmas
molecular clouds
supernovae
power law
indication
plasma
photons
temperature
interactions

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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title = "A hard extended X-ray source in the IC 443 supernova remnant resolved by Chandra: A fast ejecta fragment or a new pulsar wind nebula?",
abstract = "A Chandra observation of the isolated hard X-ray source XMMU J061804.3+222732, located in the region of the apparent interaction of the supernova remnant IC 443 with a molecular cloud, resolved the complex structure of the source in a few bright clumps embedded in an extended emission of ∼30″ in size. The X-ray spectra of the clumps and the extended emission are dominated by a hard power-law component with a photon index of 1.2-1.4. In addition, we see some indications of an optically thin thermal plasma of an ∼0.3 keV temperature. The observed X-ray morphology and spectra are consistent with those expected for an isolated supernova ejecta fragment interacting with a dense ambient medium. A possible alternative interpretation is a pulsar wind nebula associated with either IC 443 or another supernova remnant, G189.6+3.3.",
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A hard extended X-ray source in the IC 443 supernova remnant resolved by Chandra : A fast ejecta fragment or a new pulsar wind nebula? / Bykov, A. M.; Bocchino, F.; Pavlov, George.

In: Astrophysical Journal, Vol. 624, No. 1 II, 01.05.2005.

Research output: Contribution to journalArticle

TY - JOUR

T1 - A hard extended X-ray source in the IC 443 supernova remnant resolved by Chandra

T2 - A fast ejecta fragment or a new pulsar wind nebula?

AU - Bykov, A. M.

AU - Bocchino, F.

AU - Pavlov, George

PY - 2005/5/1

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N2 - A Chandra observation of the isolated hard X-ray source XMMU J061804.3+222732, located in the region of the apparent interaction of the supernova remnant IC 443 with a molecular cloud, resolved the complex structure of the source in a few bright clumps embedded in an extended emission of ∼30″ in size. The X-ray spectra of the clumps and the extended emission are dominated by a hard power-law component with a photon index of 1.2-1.4. In addition, we see some indications of an optically thin thermal plasma of an ∼0.3 keV temperature. The observed X-ray morphology and spectra are consistent with those expected for an isolated supernova ejecta fragment interacting with a dense ambient medium. A possible alternative interpretation is a pulsar wind nebula associated with either IC 443 or another supernova remnant, G189.6+3.3.

AB - A Chandra observation of the isolated hard X-ray source XMMU J061804.3+222732, located in the region of the apparent interaction of the supernova remnant IC 443 with a molecular cloud, resolved the complex structure of the source in a few bright clumps embedded in an extended emission of ∼30″ in size. The X-ray spectra of the clumps and the extended emission are dominated by a hard power-law component with a photon index of 1.2-1.4. In addition, we see some indications of an optically thin thermal plasma of an ∼0.3 keV temperature. The observed X-ray morphology and spectra are consistent with those expected for an isolated supernova ejecta fragment interacting with a dense ambient medium. A possible alternative interpretation is a pulsar wind nebula associated with either IC 443 or another supernova remnant, G189.6+3.3.

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