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Volumn 390, Issue 2, 2002, Pages 533-553

The carrier of the "30" μm emission feature in evolved stars: A simple model using magnesium sulfide

Author keywords

Circumstellar matter; Infrared: stars; Planetary nebulae: general; Stars: AGB and post AGB; Stars: carbon; Stars: mass loss

Indexed keywords

DUST; GRAIN SIZE AND SHAPE; INFRARED RADIATION; MAGNESIUM COMPOUNDS; PLANETS; THERMAL EFFECTS;

EID: 0036682109     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20020603     Document Type: Article
Times cited : (135)

References (49)
  • 9
    • 0003094441 scopus 로고
    • Astronomical Infrared Spectroscopy: Future Observational Directions
    • (1993) ASP Conf. Ser. , vol.41 , pp. 163
    • Cox, P.1
  • 35
    • 0009831260 scopus 로고
    • Astronomical Infrared Spectroscopy: Future Observational Directions
    • (1993) ASP Conf. Ser. , vol.41 , pp. 87
    • Omont, A.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.