An XMM-Newton study of hyper-luminous infrared galaxies
This paper is based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA; Chandra, a NASA mission; BeppoSAX, a project of the ASI (Italy) with participation of the NIVR (Netherlands) and the Space Science De...
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2007 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/3835 |
| Acceso en línea: | http://hdl.handle.net/10261/3835 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxies: active Galaxies: starburst Galaxies: evolution X-ray galaxies Infrared: galaxies |
| Sumario: | This paper is based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA; Chandra, a NASA mission; BeppoSAX, a project of the ASI (Italy) with participation of the NIVR (Netherlands) and the Space Science Department of ESA; ISO, an ESA project with the participation of ISAS and NASA; and IRAS, a joint project of the US, UK and the Netherlands. This research also has made use of the SuperCOSMOS Sky Survey (SSS) data base and the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. |
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