2012A&A...542A..39G -
Astronomy and Astrophysics, volume 542A, 39-39 (2012/6-1)
Star formation in grand-design, spiral galaxies. Young, massive clusters in the near-infrared.
GROSBOL P. and DOTTORI H.
Abstract (from CDS):
Spiral structure is a prominent feature in many disk galaxies and is often outlined by bright, young objects. We study the distribution of young stellar clusters in grand-design spiral galaxies and thereby determine whether strong spiral perturbations can influence star formation. Deep, near-infrared JHK-maps were observed for ten nearby, grand-design, spiral galaxies using HAWK-I at the Very Large Telescope. Complete, magnitude-limited candidate lists of star-forming complexes were obtained by searching within the K-band maps. The properties of the complexes were derived from (H-K)-(J-H) diagrams including the identification of the youngest complexes (i.e. ≲7Myr) and the estimation of their extinction. Young stellar clusters with ages ≲7Myr have significant internal extinction in the range of AV=3-7m, while older ones typically have AV<1m. The cluster luminosity function (CLF) is well-fitted by a power law with an exponent of around -2 and displays no evidence of a high luminosity cut-off. The brightest cluster complexes in the disk reach luminosities of MK=-15.5mag or estimated masses of 106M☉. At radii with a strong, two-armed spiral pattern, the star formation rate in the arms is higher by a factor of 2-5 than in the inter-arm regions. The CLF in the arms is also shifted towards brighter MK by at least 0.4.mag We also detect clusters with colors compatible with Large Magellanic Cloud intermediate age clusters and Milky Way globular clusters. The (J-K)-MK diagram of several galaxies shows, for the brightest clusters, a clear separation between young clusters that are highly attenuated by dust and older ones with low extinction. The gap in the (J-K)-MK diagrams implies that there has been a rapid expulsion of dust at an age around 7Myr, possibly triggered by supernovae. Strong spiral perturbations concentrate the formation of clusters in the arm regions and shifts their CLF towards brighter magnitudes.
Abstract Copyright:
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Journal keyword(s):
galaxies: spiral - galaxies: structure - galaxies: star clusters: general - galaxies: star formation - infrared: galaxies - techniques: photometric
VizieR on-line data:
<Available at CDS (J/A+A/542/A39): table1.dat n0157c.dat n1232c.dat n1300c.dat n1365c.dat n1566c.dat n2997c.dat n4030c.dat n4321c.dat n5247c.dat n7424c.dat>
Nomenclature:
[GD2012] NGCNNNN NNNN N=25520
Status at CDS
:
All or part of tables of objects could be ingested in SIMBAD with priority 2.
Simbad objects:
17
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