Evidence of asymmetric structure in the atmosphere of Mira variable U Orionis from lunar occultation observations in the near-infrared

Monthly Notices of the Royal Astronomical Society

Volumn 348, Issue 4, 2004, Pages 1332-1336

  Mondal, Soumen ^a   Chandrasekhar, T ^a  

^a PHYSICAL RESEARCH LABORATORY   (India)

Author keywords

Infrared: general; Occultations; Stars: individual: U Ori

Indexed keywords

ANGULAR DIAMETERS; ASYMMETRIC STRUCTURES; INFRARED: GENERAL; LUNAR OCCULTATION; MODEL INDEPENDENT; NEAR INFRARED; NEAR-INFRARED; OCCULTATION; STAR: INDIVIDUAL: U ORI; STARS: INDIVIDUAL: PROXIMA CENTAURI;

INFRARED DEVICES;

EID: 1642356505     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07454.x     Document Type: Article

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