Dust-penetrated arm classes: Insights from rising and falling rotation curves

Monthly Notices of the Royal Astronomical Society

Volumn 359, Issue 3, 2005, Pages 1065-1076

  Seigar, M S ^a,b   Block, D L ^c   Puerari, I ^d   Chorney, N E ^b,e   James, P A ^f  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF HAWAII   (United States)

^c UNIVERSITY OF THE WITWATERSRAND   (South Africa)

^d INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^e UNIVERSITY OF VICTORIA   (Canada)

^f LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

Author keywords

Galaxies: fundamental parameters; Galaxies: spiral; Galaxies: structure; Infrared: galaxies

Indexed keywords

FOURIER ANALYSIS; GALAXIES; INFRARED DEVICES; MORPHOLOGY; ROTATION; STARS; THERMOGRAPHY (IMAGING);

GALAXIES: FUNDAMENTAL PARAMETERS; GALAXIES: SPIRALS; GALAXIES:STRUCTURE; INFRARED GALAXIES; NEAR INFRARED; NEAR-INFRARED; PITCH ANGLE; ROTATION CURVES; SPIRAL ARMS; STELLAR DISKS;

DUST;

EID: 19844367168     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08970.x     Document Type: Article

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