Variations of the spectral index of dust emissivity from Hi-GAL observations of the Galactic plane

Astronomy and Astrophysics

Volumn 520, Issue 6, 2010, Pages

  Paradis, D ^a   Veneziani, M ^a,b   Noriega Crespo, A ^a   Paladini, R ^a   Piacentini, F ^b   Bernard, J P ^c,d   De Bernardis, P ^b   Calzoletti, L ^e   Faustini, F ^e   Martin, P ^f   Masi, S ^b   Montier, L ^c,d   Natoli, P ^g   Ristorcelli, I ^c,d   Thompson, M A ^h   Traficante, A ^g   Molinari, S ⁱ  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b SAPIENZA UNIVERSITY OF ROME   (Italy)

^c IRAP   (France)

^d CNRS   (France)

^e ASI SCIENCE DATA CENTER   (Italy)

^f UNIVERSITY OF TORONTO   (Canada)

^g UNIVERSITY OF ROME TOR VERGATA   (Italy)

^h UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

ⁱ INAF   (Italy)

Author keywords

Dust, extinction; Infrared: ISM

Indexed keywords

ANGULAR RESOLUTION; COSMIC MICROWAVE BACKGROUNDS; DUST , EXTINCTION; FAR-INFRARED; GALACTIC PLANE; GAS MASS; HERSCHEL; INFRARED: ISM; INNER REGION; INVERSE CORRELATION; MEDIAN VALUE; POWER LAW; SPATIAL VARIATIONS; SPECTRAL INDICES;

ELECTROMAGNETIC WAVE EMISSION;

DUST;

EID: 77957558018     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015301     Document Type: Article

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