The link between submillimetre galaxies and luminous ellipticals : near-infrared IFU spectroscopy of submillimetre galaxies
- Author
- SWINBANK, A. M1 ; CHAPMAN, S. C2 ; SMAIL, Ian1 ; LINDNER, C2 ; BORYS, C2 3 ; BLAIN, A. W2 ; IVISON, R. J4 5 ; LEWIS, G. F6
[1] Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DHI 3LE, United States
[2] Astronomy Department, California Institute of Technology, 105-24, Pasadena, CA 91125, United States
[3] University of Toronto, Toronto, Ontario M5S 3H8, Canada
[4] Astrcnomy Technology Center, Royal Observatory, Blackford Hill, Edinburgh EH19 3HJ, United Kingdom
[5] Institute for Astronomy, University of Edinburgh, Edinburgh EH19 3HJ, United Kingdom
[6] School of Physics, University of Sydney, NSW 2006, Australia - Source
Monthly Notices of the Royal Astronomical Society. 2006, Vol 371, Num 1, pp 465-476, 12 p ; ref : 62 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- galaxies: evolution galaxies: high-redshift galaxies: individual submillimetre
- Keyword (fr)
- Baryon Champ proche Durée vie Dynamique Déplacement vers le rouge Emission optique Etoile baryon Galaxies actives Galaxies elliptiques Galaxies premier type Luminosité Masse stellaire Morphologie Noyau galactique actif Noyau galaxies Population stellaire Raie émission Spectrométrie 2 dimensions Spectrométrie IR proche Spectrométrie IR Système multiple Taux formation Evolution galaxies
- Keyword (en)
- Baryons Near field Lifetime Dynamics Red shift Light emission Baryon star Active galaxies Elliptical galaxies Early type galaxies Luminosity Stellar mass Morphology Active galaxy nuclei Galaxy nuclei Stellar population Emission line Two-dimensional spectroscopy Near infrared spectrometry Infrared spectroscopy Multiple system Formation rate Galaxy evolution
- Keyword (es)
- Campo próximo Emisión óptica Estrella baritrón Galaxias primer tipo Población estelar Raya emisión Espectrometría IR próximo Sistema múltiple Grado formación Evolución galaxias
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18041515
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
10.1111/j.1365-2966.2006.10673.x 
https://dx.doi.org/10.1111/j.1365-2966.2006.10673.x
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