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
- 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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DOI
10.1086/524406 
https://dx.doi.org/10.1086/524406
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