The IR-colour-mass-loss relation of carbon-rich, dust-driven superwinds and a synthetic (J-K, MBol) diagram

Astronomy and Astrophysics

Volumn 398, Issue 1, 2003, Pages 229-237

  Schroder K P ^a,b   Wachter, A ^a,b   Winters, J M ^c,d  

^a UNIVERSITY OF SUSSEX   (United Kingdom)

^b TECHNISCHE UNIVERSITÄT BERLIN   (Germany)

^c MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^d OBSERVATOIRE DE PARIS   (France)

Author keywords

Infrared: stars; Stars: carbon; Stars: circumstellar matter; Stars: evolution; Stars: late type; Stars: mass loss

Indexed keywords

APPROXIMATION THEORY; CARBON; CORRELATION METHODS; LUMINESCENCE; MAXIMUM LIKELIHOOD ESTIMATION; PHOTOMETRY;

PLANETARY NEBULAE (PN);

ASTROPHYSICS;

EID: 0037246262     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021601     Document Type: Article

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