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A young double stellar cluster in an Hll region, emerging from its parent molecular cloud

Author
YUN, J. L1 ; DJUPVIK, A. A2 ; DELGADO, A. J3 ; ALFARO, E. J3
[1] Universidade de Lisboa -Faculdade de Ciências Centro de Astronomia e Astrofísica da Universidade de Lisboa, Observatório Astronómico de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal
[2] Nordic Optical Telescope, Apdo 474, 38700 Santa Cruz de La Palma, Spain
[3] Instituto de Astrofísica de Andalucía, CSIC, Apdo 3004, 18080-Granada, Spain
Source

Astronomy and astrophysics (Berlin. Print). 2008, Vol 483, Num 1, pp 209-221, 13 p ; ref : 3/4 p

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
ISM: HII regions ISM: dust, extinction ISM: individual objects: IRAS 07141-0920 ISM: individual objects: Sh2-294 (S294) stars: formation stars: pre-main sequence
Keyword (fr)
Age Amas jeune Amas stellaire Complexité Diagramme magnitude couleur Etoile massive Excès IR Formation stellaire Isochrone Jet Lumière diffuse Nuage moléculaire Nébuleuse émissive Photométrie Région HII Source ponctuelle
Keyword (en)
Age Young cluster Star clusters Complexity Color-magnitude diagrams Massive stars Infrared excess Star formation Isochrone Jets Scattered light Molecular clouds Emission nebulae Photometry HII regions Point sources
Keyword (es)
Edad Cúmulo joven Complejidad Exceso IR Isocrono Luz difusa
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20327650

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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