Age distributions of star clusters in spiral and barred galaxies as a test for theories of spiral structure

We consider models of gas flow in spiral galaxies in which the spiral structure has been excited by various possible mechanisms: a global steady density wave, self-gravity of the stellar disc and an external tidal interaction, as well as the case of a galaxy with a central rotating bar. In each mode...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2010-11, Vol.409 (1), p.396-404
Main Authors: Dobbs, C. L., Pringle, J. E.
Format: Article
Language:English
Subjects:
Astronomy
Earth, ocean, space
Exact sciences and technology
galaxies: kinematics and dynamics
galaxies: spiral
galaxies: star clusters: general
galaxies: star formation
galaxies: structure
Gravity
Stars & galaxies
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Summary:We consider models of gas flow in spiral galaxies in which the spiral structure has been excited by various possible mechanisms: a global steady density wave, self-gravity of the stellar disc and an external tidal interaction, as well as the case of a galaxy with a central rotating bar. In each model we estimate in a simple manner the likely current positions of star clusters of a variety of ages, ranging from ∼2 to around ∼130 Myr, depending on the model. We find that the spatial distribution of clusters of different ages varies markedly depending on the model, and propose that observations of the locations of age-dated stellar clusters is a possible discriminant between excitation mechanisms for spiral structure in an individual galaxy.
ISSN:0035-8711
1365-2966
DOI:10.1111/j.1365-2966.2010.17323.x