Long-term evolution of FU Orionis objects at infrared wavelengths

Astronomy and Astrophysics

Volumn 428, Issue 1, 2004, Pages 89-97

  Abraham P ^a   Kospal A ^b   Csizmadia, Sz ^a   Kun, M ^a   Moor A ^a   Prusti, T ^c  

^a KONKOLY OBSERVATORY   (Hungary)

^b EÖTVÖS LORÁND UNIVERSITY   (Hungary)

^c EUROPEAN SPACE AGENCY   (Netherlands)

Author keywords

Infrared: stars; Stars: circumstellar matter; Stars: individual: V1057 Cyg; Stars: pre main sequence

Indexed keywords

DATA PROCESSING; INFRARED RADIATION; PHOTOMETRY; PROJECT MANAGEMENT; SPECTRUM ANALYSIS; SUBLIMATION;

INFRARED: STARS; STARS: CIRCUMSTELLAR MATTER; STARS: INDIVIDUAL: V1057 CYG; STARS: PRE-MAIN SEQUENCE;

ASTRONOMY;

EID: 10044252288     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040315     Document Type: Article

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