Where are the stars of the bar of NGC 1530 forming?

Astronomy and Astrophysics

Volumn 485, Issue 1, 2008, Pages 5-20

  Zurita, A ^a,b   Perez I ^a,b,c  

^a UNIVERSITY OF GRANADA   (Spain)

^b Instituto Carlos I de Física Teórica y Computacional   (Spain)

^c UNIVERSITY OF GRONINGEN   (Netherlands)

Author keywords

Galaxies: individual: NGC 1530; galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: spiral; Galaxies: structure; ISM: HII regions

Indexed keywords

DYNAMICS; EQUIVALENCE CLASSES; FORMING; IONIZING RADIATION; MECHANICS; METALLIZING; NICKEL COMPOUNDS; PHOTOMETRY; RADIATION; STARS;

(I ,J) CONDITIONS; AGE DIFFERENCES; BAR DYNAMICS; BROAD BANDS; DYNAMICAL FEATURES; GAS FLOWING; H II REGIONS; MAJOR AXIS; MASSIVE STARS; MAXIMUM VELOCITY; METALLICITY; NGC 1530; PHOTOMETRIC PROPERTIES; SPATIAL CORRELATION (SC); SPATIAL RELATIONS; STAR FORMATION (SF); TIME SCALING;

DUST;

EID: 45249086129     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079129     Document Type: Article

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