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A HALF-MEGASECOND CHANDRA OBSERVATION OF THE OXYGEN-RICH SUPERNOVA REMNANT G292.0+1.8

Author
PARK, Sangwook1 ; HUGHES, John P2 3 ; SLANE, Patrick O4 ; BURROWS, David N1 ; GAENSLER, B. M5 ; GHAVAMIAN, Parviz6
[1] Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, United States
[2] Department of Physics and Astronomy, Rutgers University, 136 Freling-huysen Road, Piscataway, NJ 08854-8019, United States
[3] Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544-1001, United States
[4] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, United States
[5] School of Physics, University of Sydney, NSW 2006, Australia
[6] Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, United States
Source

The Astrophysical journal. 2007, Vol 670, Num 2 ; L121-L124 ; 2 ; ref : 1/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
ISM: individual (G292.0+1.8)-pulsars: individual (J1124-5916)- supernova remnants X-rays: ISM
Keyword (fr)
Pulsar Reste supernova
Keyword (en)
Pulsars Supernova remnants
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19893868

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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