Modelling the spinning dust emission from dense interstellar clouds

Astronomy and Astrophysics

Volumn 535, Issue , 2011, Pages

  Ysard, N ^a   Juvela, M ^a   Verstraete, L ^b  

^a UNIVERSITY OF HELSINKI   (Finland)

^b UNIVERSITÉ PARIS SUD   (France)

Author keywords

dust, extinction; evolution; ISM: clouds; ISM: general; radiative transfer

Indexed keywords

DENSE MEDIA; DENSE MEDIUM; DENSE MOLECULAR CLOUD; DIFFUSE INTERSTELLAR MEDIUMS; DUST , EXTINCTION; DUST EMISSION; ELECTRIC-DIPOLE EMISSION; EVOLUTION; GAS STATE; INTERSTELLAR CLOUDS; ISM : CLOUDS; ISM: GENERAL; MAJOR IONS; MICROWAVE EMISSIONS; MID-IR EMISSIONS; PAH EMISSIONS; PHYSICAL CONDITIONS; RADIATIVE TRANSFER SIMULATIONS;

CLOUDS; EMISSION SPECTROSCOPY; ESTIMATION; GRAIN GROWTH; HYDROCARBONS; MICROWAVES; POLYCYCLIC AROMATIC HYDROCARBONS; RADIATIVE TRANSFER; TRACE ANALYSIS;

DUST;

EID: 81355151236     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117394     Document Type: Article

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