Towards a spectral technique for determining material geometry around evolved stars: Application to HD 179821

Monthly Notices of the Royal Astronomical Society

Volumn 388, Issue 2, 2008, Pages 716-722

  Nordhaus, J ^a,b   Minchev, I ^a   Sargent, B ^a   Forrest, W ^a   Blackman, E G ^a,b   De Marco, O ^c   Kastner, J ^d   Balick, B ^e   Frank, A ^a,b  

^a UNIVERSITY OF ROCHESTER   (United States)

^b UNIVERSITY OF ROCHESTER   (United States)

^c DIVISION OF INVERTEBRATE ZOOLOGY   (United States)

^d ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

^e UNIVERSITY OF WASHINGTON   (United States)

Author keywords

Circumstellar matter; Infrared: general; Planetary nebulae: general; Radiative transfer; Stars: AGB and post AGB; Submillimetre

Indexed keywords

CODES (SYMBOLS); DUST; GEOMETRY; STARS;

BROAD BANDS; CENTRAL SOURCE; CIRCUMSTELLAR MATTERS; EVOLVED STARS; INFRARED: GENERAL; PLANETARY NEBULAE:GENERAL; SPECTRAL ENERGY DISTRIBUTION; STARS:AGB AND POST AGB; SUBMILLIMETRE; SYMMETRICS;

RADIATIVE TRANSFER;

EID: 47649091451     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13428.x     Document Type: Article

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