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The origin of the hot metal-poor gas in NGC 1291 : Testing the hypothesis of gas dynamics as the cause of the gas heating

Author
PEREZ, I1 ; FREEMAN, K2
[1] Kapteyn Astronomical Institute, University of Groningen, Postbus 800, Groningen 9700 AV, Netherlands
[2] RSAA, Mount Stromlo Observatory, Cotter road, Weston Creek, ACT 2611, Australia
Source

Astronomy and astrophysics (Berlin. Print). 2006, Vol 454, Num 1, pp 165-169, 5 p ; ref : 17 ref

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
Galaxy: abundances X-rays: galaxies galaxies: ISM galaxies: kinematics and dynamics galaxies: structure
Keyword (fr)
Abondance Cinématique Couleur Dynamique gaz Galaxies RX Gaz chaud Métallicité Raie émission Région HII Source RX cosmique Spectrométrie Structure galaxies
Keyword (en)
Abundance Kinematics Color Gas dynamics X-ray galaxies Hot gas Metallicity Emission line HII regions Cosmic x-ray sources Spectroscopy Galaxy structure
Keyword (es)
Gas caliente Metalicidad Raya emisión Estructura galaxias
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17920502

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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