Dust-correlated cm wavelength continuum emission from translucent clouds ζ Oph and LDN 1780

Monthly Notices of the Royal Astronomical Society

Volumn 414, Issue 3, 2011, Pages 2424-2435

  Vidal, M ^a,b   Casassus, S ^b,c   Dickinson, C ^a   Witt, A N ^d   Castellanos, P ^b   Davies, R D ^a   Davis, R J ^a   Cabrera, G ^b   Cleary, K ^e   Allison, J R ^f   Bond, J R ^g   Bronfman, L ^b   Bustos, R ^b,h   Jones, M E ^f   Paladini, R ⁱ   Pearson, T J ^e   Readhead, A C S ^e   Reeves, R ^h   Sievers, J L ^g   Taylor, A C ^f  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b UNIVERSITY OF CHILE   (Chile)

^c OBSERVATOIRE DE PARIS   (France)

^d UNIVERSITY OF TOLEDO   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f UNIVERSITY OF OXFORD   (United Kingdom)

^g UNIVERSITY OF TORONTO   (Canada)

^h UNIVERSITY OF CONCEPCIÓN   (Chile)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

ISM: individual objects: LDN 1780; ISM: individual objects: Ophiuchi; Radiation mechanisms: general; Radio continuum: ISM

Indexed keywords

COSMOLOGY; DUST; ELECTROMAGNETIC WAVE EMISSION; INFRARED IMAGING;

ANGULAR SCALE; CIRRUS CLOUDS; COSMICS; ISM: INDIVIDUAL OBJECT: LDN 1780; ISM: INDIVIDUAL OBJECT: Ζ OPHIUCHI; ISM: INDIVIDUAL OBJECTS; RADIATION MECHANISMS: GENERAL; RADIO CONTINUUM: ISM; TRANSLUCENTS;

CLOUDS;

EID: 79959378745     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18562.x     Document Type: Article

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