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RESOLVING THE ELECTRON TEMPERATURE DISCREPANCIES IN H II REGIONS AND PLANETARY NEBULAE: κ-DISTRIBUTED ELECTRONS

Author
NICHOLLS, David C1 ; DOPITA, Michael A1 2 ; SUTHERL, Ralph S1
[1] Research School of Astronomy and Astrophysics, Australian National University, Cotter Rd., Weston ACT 2611, Australia
[2] Astronomy Department, King Abdulaziz University, P.O. Box 80203, Jeddah, Saudi Arabia
Source

The Astrophysical journal. 2012, Vol 752, Num 2 ; 752148.1-752148.16 ; 1 ; ref : 1/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
IOP, Bristol
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
H II regions ISM: abundances acceleration of particles atomic data atomic processes planetary nebulae: general plasmas
Keyword (fr)
Abondance Accélération particule Métallicité Nébuleuse gazeuse Nébuleuse planétaire Plasma solaire Processus atomique Région HII Système solaire Température électron Voie lactée
Keyword (en)
Abundance Particle acceleration Metallicity Gaseous nebulae Planetary nebulae Solar plasma Atomic process HII regions Solar system Electron temperature Milky Way
Keyword (es)
Aceleración partícula Metalicidad Plasma solar Proceso atómico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
26017317

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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