A multi-wavelength analysis of M 81: Insight on the nature of Arp's loop

Astronomy and Astrophysics

Volumn 516, Issue 22, 2010, Pages

  Sollima, A ^a   Gil De Paz, A ^b   Martinez Delgado, D ^a,c   Gabany, R J ^d   Gallego Laborda, J J ^e   Hallas, T ^f  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSIDAD COMPLUTENSE DE MADRID   (Spain)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^d Blackbird Observatory   (United States)

^e Fosca Nit Observatory   (Spain)

^f Hallas Observatory Annex   (United States)

Author keywords

galaxies: individual: M 81; infrared: galaxies; methods: data analysis; techniques: photometric

Indexed keywords

CLOUDS; COMPLEXATION; DATA REDUCTION; DISKS (STRUCTURAL COMPONENTS); DUST; DYES; GALAXIES; GEOMETRICAL OPTICS; INFRARED IMAGING; PHOTOMETRY; PLASMA WAVES;

COLD DUST; FAR-INFRARED; FILAMENTARY STRUCTURES; GALAXIES: INDIVIDUAL: M 81; GAS RATIO; INFRARED EMISSIONS; INFRARED IMAGES; INFRARED: GALAXIES; METHODS: DATA ANALYSIS; MULTIWAVELENGTH; OPTICAL IMAGE; OPTICAL RINGS; OPTICAL WAVELENGTH; SCATTERED LIGHT; SPITZER; STAR-FORMING REGION; TECHNIQUES: PHOTOMETRIC; TIDAL INTERACTIONS; WIDE-FIELD;

INTERNET PROTOCOLS;

EID: 77957881753     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014085     Document Type: Article

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