Modelling the optical properties of composite and porous interstellar grains

Astronomy and Astrophysics

Volumn 429, Issue 2, 2005, Pages 371-381

  Voshchinnikov, N V ^a,b   Il'in, V B ^a,b   Henning, Th ^c  

^a ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^b Isaac Newton Institute of Chile   (Russian Federation)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Extinction Comets Interplanetary medium; Scattering Dust

Indexed keywords

APPROXIMATION THEORY; COSMIC RAYS; CRYSTAL MICROSTRUCTURE; DUST; ELECTROMAGNETIC WAVE SCATTERING; GRAPHITE; MATHEMATICAL MODELS; POROSITY; SILICATES;

COMETS; DUST, EXTINCTION; EFFECTIVE MEDIUM THEORIS (EMT); INTERPLANETARY MEDIUM;

ASTROPHYSICS;

EID: 11144238079     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:200400081     Document Type: Article

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