Modelling near-IR spectra and mid-IR dust emission of Mira variables at different phases

Monthly Notices of the Royal Astronomical Society

Volumn 317, Issue 2, 2000, Pages 391-405

  Lobel, A ^a   Bagnulo, S ^b   Doyle, J G ^c   Power, C ^c  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY OF VIENNA   (Austria)

^c ARMAGH OBSERVATORY   (United Kingdom)

Author keywords

Circumstellar matter; Infrared: stars; Stars: AGB and post AGB; Stars: individual: o Cet; Stars: individual: U Ori; Stars: variables: other

Indexed keywords

SILICATES; SPECTROSCOPY; STARS; TEMPERATURE;

CIRCUMSTELLAR MATTERS; DUST EMISSION; INFRARED: STAR; STAR: INDIVIDUAL: O CET; STAR: INDIVIDUAL: U ORI; STAR: VARIABLE: OTHER; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: VARIABLES; STARS:AGB AND POST AGB;

DUST;

EID: 0000325869     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03563.x     Document Type: Article

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