Further evidence for the FU Orionis nature of PP 13S

Monthly Notices of the Royal Astronomical Society

Volumn 328, Issue 3, 2001, Pages 751-761

  Aspin, Colin ^a,c   Sandell, Göran ^b  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b NASA AMES RESEARCH CENTER   (United States)

^c GEMINI OBSERVATORY   (United States)

Author keywords

ISM: jets and outflows; Stars: formation; Stars: individual: PP 13S; Stars: mass loss; Stars: pre main sequence

Indexed keywords

INFRARED DEVICES; INFRARED IMAGING;

INFRARED: SPECTROSCOPY; ISM JETS AND OUTFLOWS; NEAR- INFRARED IMAGES; OPTICAL-; STAR: INDIVIDUAL: PP 13S; STARS FORMATION; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MASS-LOSS; STARS: PRE-MAIN SEQUENCE; SUBMILLIMETRE;

STARS;

EID: 0041735288     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04687.x     Document Type: Article

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