2MASS wide field extinction maps: III. the taurus, perseus, and california cloud complexes

Astronomy and Astrophysics

Volumn 512, Issue 10, 2010, Pages

  Lombardi, M ^a,b   Lada, C J ^c   Alves, J ^d  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b UNIVERSITY OF MILAN   (Italy)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d CENTRO ASTRONÓMICO HISPANO ALEMÁN   (Spain)

Author keywords

Dust; Extinction; ISM: clouds; ISM: individual objects: Taurus molecular complex; ISM: structure; Methods: statistical

Indexed keywords

DUST; GEOMETRICAL OPTICS; INFRARED DEVICES; NORMAL DISTRIBUTION; STARS; TURBULENCE MODELS;

23 MILLION; ALL-SKY SURVEY; CALIFORNIA; CLOUD STRUCTURE; COLUMN DENSITY; EXTINCTION VALUES; EXTINCTION-ISM; GALACTIC PLANE; ISM: STRUCTURE; LARGE REGIONS; LARGE-SCALE STRUCTURE; LOG-NORMAL DISTRIBUTION; METHODS:STATISTICAL; MOLECULAR CLOUDS; MOLECULAR COMPLEXES; NEAR INFRARED; NEAR-INFRARED WAVELENGTH; OPTIMAL METHODS; POINT SOURCES; TURBULENT MODELS; WIDE FIELD;

CLOUDS;

EID: 77951556216     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912670     Document Type: Article

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