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2MASS wide field extinction maps: III. The Taurus, Perseus, and California cloud complexes

Author
LOMBARDI, M1 2 ; LADA, C. J3 ; ALVES, J4
[1] European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany
[2] University of Milan, Department of Physics, via Celoria 16, 20133 Milan, Italy
[3] Harvard-Smithsonian Center for Astrophysics, Mail Stop 72, 60 Garden Street, Cambridge, MA 02138, United Kingdom
[4] Calar Alto Observatory - Centro Astronómico Hispano Alemán, C/Jesús Durbán Remón 2-2, 04004 Almeria, Spain
Source

Astronomy and astrophysics (Berlin. Print). 2010, Vol 512 ; 512A67.1-512A67.14 ; ref : 1/4 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: clouds ISM: individual objects: Taurus molecular complex ISM: structure dust, extinction methods: statistical
Keyword (fr)
Catalogue astronomique Densité colonne Etude ciel Fonction structure Gravité Loi lognormale Modèle Méthode statistique Nuage moléculaire Plan galactique Source ponctuelle Structure grande échelle Turbulence
Keyword (en)
Astronomical catalogues Column density Sky surveys Structure functions Gravity Log normal distribution Models Statistical method Molecular clouds Galactic planes Point sources Large-scale structure Turbulence
Keyword (es)
Densidad columna Modelo Método estadístico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
22835144

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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