Hydrogen 21-centimeter emission from a galaxy at cosmological distance
- Autor
- ZWAAN, M. A1 ; VAN DOKKUM, P. G2 ; VERHEIJEN, M. A. W3 4
[1] School of Physics, University of Melbourne, Victoria 3010, Australia
[2] California Institute of Technology, Mail Stop 105-24, Pasadena, CA 91125, United States
[3] Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706, United States
[4] National Radio Astronomical Observatory, Post Office Box 0, Socorro, NM 87801, United States - Fuente
Science (Washington, D.C.). 2001, Vol 293, Num 5536, pp 1800-1802 ; ref : 31 ref
- CODEN
- SCIEAS
- ISSN
- 0036-8075
- Campo Científico
- Multidisciplinary
- Editor
- American Association for the Advancement of Science, Washington, DC
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Amas galaxies Galaxies spirales Modèle cosmologique Observation radio Raie 21 cm Raie H Raie émission Taux accrétion Abell 2218
- Palabra clave (in)
- Galaxy clusters Spiral galaxies Cosmological models Radio observation 21cm-Line H lines Emission line Accretion rate
- Palabra clave (es)
- Observación radio Raya 21 cm Raya emisión Índice acreción
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D52 Normal galaxies. Extragalactic objects and systems (by type) / 001E03D52N Spiral galaxies
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D58 Interstellar medium (ism) and nebulae in external galaxies / 001E03D58G H i regions and 21-cm lines ; diffuse, translucent, and high-velocity clouds
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D65 Galaxy groups, clusters, and superclusters. Large-scale structure of the universe / 001E03D65C Galaxy clusters
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 1116586
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
10.1126/science.1063034 
https://dx.doi.org/10.1126/science.1063034
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