Modeling optical properties of cosmic dust grains using a distribution of hollow spheres

Astronomy and Astrophysics

Volumn 432, Issue 3, 2005, Pages 909-920

  Min, M ^a   Hovenier, J W ^a   De Koter, A ^a  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

Author keywords

Infrared: general; Polarisation; Scattering; Stars: circumstellar matter

Indexed keywords

ABSORPTION; COMPUTATIONAL METHODS; COMPUTER SIMULATION; COSMIC RAYS; INFRARED SPECTROSCOPY; LIGHT EMISSION; LIGHT POLARIZATION; LIGHT SCATTERING; MATRIX ALGEBRA; NUMERICAL ANALYSIS; PARTICLE SIZE ANALYSIS; PARTICLES (PARTICULATE MATTER); POROSITY;

CIRCUMSTELLAR MATTERS-INFRARED; DEGREE OF LINEAR POLARIZATION; DISTRIBUTION OF HOLLOW SPHERES; GENERAL; POLARIZATION-SCATTERING-STARS; SCATTERING ANGLE DISTRIBUTION;

ASTROPHYSICS;

EID: 15544389191     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041920     Document Type: Article

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