TIMING AND SPECTRAL PROPERTIES OF THE ACCRETING MILLISECOND PULSAR SWIFT J1756.9-2508
- Author
- LINARES, Manuel1 ; WIJNANDS, Rudy1 ; VAN DER KLIS, Michiel1 ; KRIMM, Hans2 3 ; MARKWARDT, Craig B2 4 ; CHAKRABARTY, Deepto5
[1] Astronomical Institute Anton Pannekoek, University of Amsterdam; and Center for High-Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, Netherlands
[2] CRESST and NASA Goddard Space Flight Center, Greenbelt, MD 20771, United States
[3] Universities Space Research Association, 10211 Wincopin Circle, Suite 500, Columbia, MD 21044, United States
[4] Department of Astronomy, University of Maryland, College Park, MD 20742, United States
[5] Department of Physics and Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology, Cambridge, MA 02139, United States - Source
The Astrophysical journal. 2008, Vol 677, Num 1, pp 515-519, 5 p ; 1 ; 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
- X-rays: binaries binaries: close pulsars: individual (SWIFT J1756.9-2508) stars: neutron
- Keyword (fr)
- Binaire RX Binaire serrée Etoile neutron Propriété spectrale Pulsar milliseconde Source RX binaire Source RX cosmique Timing
- Keyword (en)
- X-ray binary stars Close binary stars Neutron stars Spectral properties Millisecond pulsar Binary X ray source Cosmic x-ray sources Timing
- Keyword (es)
- Propiedad espectral Pulsar milisegundo Fuente RX binaria
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20272197
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
10.1086/533498 
https://dx.doi.org/10.1086/533498
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