The nature of the KW object

Astronomy and Astrophysics

Volumn 427, Issue 3, 2004, Pages 849-853

  Chini, R ^a   Hoffmeister, V H ^a   Kampgen K ^a   Kimeswenger, S ^b   Nielbock, M ^a   Siebenmorgen, R ^c  

^a RUHR UNIVERSITY BOCHUM   (Germany)

^b UNIVERSITY OF INNSBRUCK   (Austria)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Galaxy: open clusters and associations: general; Infrared: stars; Stars: circumstellar matter; Stars: formation; Stars: pre main sequence

Indexed keywords

ABSORPTION; DUST; ESTIMATION; GALAXIES; INFRARED RADIATION; MATHEMATICAL MODELS; MORPHOLOGY; PHOTOMETRY; SILICATES; X RAY ANALYSIS;

GALAXY:OPEN CLUSTERS AND ASSOCIATIONS:GENERAL; INFRARED:STARS; STARS:CIRCUMSTELLAR MATTER; STARS:FORMATION; STARS:PRE-MAIN SEQUENCE;

ASTRONOMY;

EID: 10044293981     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041713     Document Type: Article

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