Observable effects of dust formation in dynamic atmospheres of M-type Mira variables

Monthly Notices of the Royal Astronomical Society

Volumn 367, Issue 4, 2006, Pages 1585-1593

  Ireland, M J ^a,c   Scholz, M ^a,b  

^a UNIVERSITY OF SYDNEY   (Australia)

^b UNIVERSITY OF HEIDELBERG   (Germany)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Stars: AGB and post AGB; Stars: variables: other; Techniques: interferometric

Indexed keywords

INTERFEROMETRY; IRON COMPOUNDS; SILICATES; STARS;

DUST FORMATION; INTERFEROMETRIC PROPERTIES; MODEL ATMOSPHERE; PHOTOMETRIC PROPERTIES; SELF CONSISTENT MODELING; STAR: VARIABLE: OTHER; STARS: VARIABLES; STARS:AGB AND POST AGB; TECHNIQUE: INTERFEROMETRIC; TEMPERATURE DEPENDENT;

DUST;

EID: 33645653054     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10064.x     Document Type: Article

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