The ISO Long Wavelength Spectrometer line spectrum of VY Canis Majoris and other oxygen-rich evolved stars

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Polehampton, E T ^a,b,c   Menten, K M ^a   Van Der Tak, F F S ^a,d   White, G J ^b,e  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^c UNIVERSITY OF LETHBRIDGE   (Canada)

^d SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^e OPEN UNIVERSITY   (United Kingdom)

Author keywords

Circumstellar matter; Stars: AGB and post AGB; Stars: individual: VY Canis Majoris; Supergiants

Indexed keywords

CIRCUMSTELLAR ENVELOPES; CIRCUMSTELLAR MATTERS; CO LINE; COLUMN DENSITY; DIAGRAM ANALYSIS; EVOLVED STARS; FAR INFRARED SPECTRUM; FITTING METHOD; HERSCHEL; HERSCHEL HIFI; LINE SPECTRA; LONG WAVELENGTH SPECTROMETER; LOWER LIMITS; MASS LOSS RATE; ORDER OF MAGNITUDE; OXYGEN CARRIER; ROTATIONAL TEMPERATURE; SIGNAL TO NOISE; SIMPLE ROTATION; SPECTRAL LINE; SPECTRAL RANGE; STARS: AGB AND POST-AGB; STARS: INDIVIDUAL: VY CANIS MAJORIS; SUPERGIANTS; VIBRATIONALLY EXCITED; WATER COLUMNS; WATER LINE; WEIGHTING SCHEME;

EXCITED STATES; OXYGEN; ROTATION; SPECTROMETERS; SPECTROMETRY; SPECTROSCOPY; WATER PIPING SYSTEMS; WATER SUPPLY;

STARS;

EID: 79952825143     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913310     Document Type: Article

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