Variations in 24-μm morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: New insights into the Hubble sequence

Monthly Notices of the Royal Astronomical Society

Volumn 380, Issue 4, 2007, Pages 1313-1334

  Bendo, G J ^a   Calzetti, D ^b   Engelbracht, C W ^c   Kennicutt, R C ^d   Meyer, M J ^e   Thornley, M D ^f   Walter, F ^g   Dale, D A ^h   Li, A ⁱ   Murphy, E J ^j  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF MASSACHUSETTS   (United States)

^c UNIVERSITY OF ARIZONA   (United States)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^e AURA for the European Space Agency   (United States)

^f BUCKNELL UNIVERSITY   (United States)

^g MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^h UNIVERSITY OF WYOMING   (United States)

ⁱ UNIVERSITY OF MISSOURI   (United States)

^j YALE UNIVERSITY   (United States)

more..

Author keywords

Galaxies: ISM; Galaxies: structure; Infrared: galaxies

Indexed keywords

DUST; STARS; SURVEYS;

CENTRALISED; DUST EMISSION; GALAXIES: ISM; GALAXIES:STRUCTURE; INFRARED GALAXIES; MORPHOLOGICAL PARAMETERS; SPITZER; STARS FORMATION; STELLARS; WAVEBANDS;

GALAXIES;

EID: 34748894839     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12204.x     Document Type: Article

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