Modelling the astronomical silicate features - I. On the spectrum subtraction method

Monthly Notices of the Royal Astronomical Society

Volumn 334, Issue 4, 2002, Pages 840-846

  Li, Aigen ^a,b,c   Greenberg, J Mayo ^d   Zhao, Gang ^a  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b PRINCETON UNIVERSITY OBSERVATORY   (United States)

^c UNIVERSITY OF ARIZONA   (United States)

^d LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Dust, extinction; Infrared: ISM; ISM: lines and bands; Scattering

Indexed keywords

CHEMICAL ANALYSIS; COMETS; SILICATE MINERALS; STARS;

ABSORPTIVITIES; ADDITIVITY; CIRCUMSTELLAR; DUST EXTINCTIONS; INFRARED: ISM; ISM: LINE AND BANDS; SPECTRA'S; SPECTRUM SUBTRACTIONS; SUBSTANTIAL ERRORS; SUBTRACTION METHOD;

ERRORS;

EID: 0041814601     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05562.x     Document Type: Article

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