X-Ray Observations of the New Pulsar-Supernova Remnant System PSR J1119–6127 and Supernova Remnant G292.2–0.5

doi:10.1086/321340

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M. J. Pivovaroff et al. 2001 ApJ 554 161 doi:10.1086/321340

X-Ray Observations of the New Pulsar-Supernova Remnant System PSR J1119–6127 and Supernova Remnant G292.2–0.5

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M. J. Pivovaroff^1,2, V. M. Kaspi^1,3,4, F. Camilo⁵, B. M. Gaensler^1,6 and F. Crawford^1,7

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mjp@space.mit.edu bmg@space.mit.edu vkaspi@physics.mcgill.ca fernando@astro.columbia.edu crawford@space.mit.edu

¹ Department of Physics and Center for Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139
² Current address: Therma-Wave, Inc., 1250 Reliance Way, Fremont, CA 94539
³ Department of Physics, Rutherford Physics Building, McGill University, 3600 University Street, Montreal, QC H3A 2T8, Canada
⁴ Alfred P. Sloan Research Fellow
⁵ Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027
⁶ Hubble Fellow
⁷ Current address: Management and Data Systems Division, Lockheed Martin Corporation, P.O. Box 8048, Philadelphia, PA 19101

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Abstract References Cited By

[1]: Observations of Energetic High Magnetic Field Pulsars with the Fermi Large Area Telescope
D. Parent et al. The Astrophysical Journal 2011 743 170
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[2]: Using Chandra to Unveil the High-Energy Properties of the High Magnetic Field Radio Pulsar J1119–6127
Samar Safi-Harb and Harsha S. Kumar The Astrophysical Journal 2008 684 532
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[3]: Unusual Pulsed X-Ray Emission from the Young, High Magnetic Field Pulsar PSR J1119–6127
M. E. Gonzalez et al. The Astrophysical Journal 2005 630 489
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[4]: Spatially Resolved Spectroscopy of the Chandra Field Containing the Supernova Remnant G292.2–0.5
Marjorie Gonzalez and Samar Safi-Harb The Astrophysical Journal 2005 619 856
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[5]: Young Core-Collapse Supernova Remnants and Their Supernovae
Roger A. Chevalier The Astrophysical Journal 2005 619 839
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[6]: Chandra Detection of the High Magnetic Field Radio Pulsar J1119–6127in the Supernova Remnant G292.2–0.5
Marjorie Gonzalez and Samar Safi-Harb The Astrophysical Journal Letters 2003 591 L143
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[7]: XMM-Newton Observations of PSR B1823–13: An Asymmetric Synchrotron Nebula around a Vela-like Pulsar
B. M. Gaensler et al. The Astrophysical Journal 2003 588 441
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[8]: PSR J1124–5916: Discovery of a Young Energetic Pulsar in the Supernova Remnant G292.0+1.8
F. Camilo et al The Astrophysical Journal Letters 2002 567 L71
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[9]: PSR J1016–5857: A Young Radio Pulsar with Possible Supernova Remnant, X-Ray, and Gamma-Ray Associations
F. Camilo et al The Astrophysical Journal Letters 2001 557 L51
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[10]: A Radio Supernova Remnant Associated with the Young Pulsar J1119–6127
Fronefield Crawford et al. The Astrophysical Journal 2001 554 152
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The Astrophysical Journal

The Astrophysical Journal

X-Ray Observations of the New Pulsar-Supernova Remnant System PSR J1119–6127 and Supernova Remnant G292.2–0.5

Observations of Energetic High Magnetic Field Pulsars with the Fermi Large Area Telescope

Using Chandra to Unveil the High-Energy Properties of the High Magnetic Field Radio Pulsar J1119–6127

Unusual Pulsed X-Ray Emission from the Young, High Magnetic Field Pulsar PSR J1119–6127

Spatially Resolved Spectroscopy of the Chandra Field Containing the Supernova Remnant G292.2–0.5

Young Core-Collapse Supernova Remnants and Their Supernovae

Chandra Detection of the High Magnetic Field Radio Pulsar J1119–6127in the Supernova Remnant G292.2–0.5

XMM-Newton Observations of PSR B1823–13: An Asymmetric Synchrotron Nebula around a Vela-like Pulsar

PSR J1124–5916: Discovery of a Young Energetic Pulsar in the Supernova Remnant G292.0+1.8

PSR J1016–5857: A Young Radio Pulsar with Possible Supernova Remnant, X-Ray, and Gamma-Ray Associations

A Radio Supernova Remnant Associated with the Young Pulsar J1119–6127

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