On the physical model of dust around Wolf-Rayet stars

Monthly Notices of the Royal Astronomical Society

Volumn 295, Issue 1, 1998, Pages 109-118

  Zubko, V G ^a,b,c  

^a NICOLAUS COPERNICUS UNIVERSITY   (Poland)

^b NATIONAL ACADEMY OF SCIENCES OF UKRAINE   (Ukraine)

^c TECHNION ISRAEL INSTITUTE OF TECHNOLOGY   (Israel)

Author keywords

Circumstellar matter; Dust, extinction; Infrared: stars; Methods: numerical; Stars: carbon; Stars: Wolf Rayet

Indexed keywords

AMORPHOUS CARBON; NUMERICAL METHODS; STARS;

CIRCUMSTELLAR MATTERS; DUST EXTINCTIONS; ELECTRICAL CHARGES; INFRARED SPECTRUM; INFRARED: STAR; METHOD: NUMERICAL; PHYSICAL MODELLING; STARS: WOLF-RAYET; STARS:CARBON; WOLF-RAYET STARS;

DUST;

EID: 0039478248     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.29511348.x     Document Type: Article

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