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Physico-chemical spectroscopic mapping of the planetary nebula NGC 40 and the 2D_NEB, a new 2D algorithm to study ionized nebulae

Author
LEAL-FERREIRA, M. L1 ; GONCALVES, D. R1 ; MONTEIRO, H2 3 ; RICHARDS, J. W4 5
[1] UFRJ ― Observatório do Valongo, Ladeira Pedro Antônio 43, 20080-090 Rio de Janeiro, RJ, Brazil
[2] Núcleo de Astrofísica Teórica-CETEC-UNICSUL, Rua Galvão Bueno, 868, 01506-000 São Paulo, SP, Brazil
[3] Universidade Federal de Itajubá, Av. BPS, 1303 Itajubá, MG, Brazil
[4] Astronomy Department, 601 Campbell Hall, University of California Berkeley, Berkeley, CA 94720, United States
[5] Statistics Department, 367 Evans Hall, University of California Berkeley, Berkeley, CA 94720, United States
Source

Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 411, Num 2, pp 1395-1408, 14 p ; ref : 1/2 p

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Wiley-Blackwell, Malden, MA
Publication country
United States
Document type
Article
Language
English
Author keyword
ISM: abundances methods: data analysis planetary nebulae: individual: NGC 40 techniques: spectroscopic
Keyword (fr)
Abondance Algorithme Analyse donnée Analyse spatiale Densité électron Nébuleuse planétaire Paramètre physique Propriété chimique Propriété physique Variation spatiale
Keyword (en)
Abundance Algorithms Data analysis Spatial analysis Electron density Planetary nebulae Physical parameter Chemical properties Physical properties Spatial variation
Keyword (es)
Análisis espacial Parámetro físico Variación espacial
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
23850988

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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