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The NGC 5253 star cluster system - I. Standard modelling and infrared-excess sources
Stockholm University, Faculty of Science, Department of Astronomy. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
Stockholm University, Faculty of Science, Department of Astronomy. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
2013 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 431, no 3, 2917-2932 p.Article in journal (Refereed) Published
Abstract [en]

Using high-resolution Hubble Space Telescope data, we re-examine the fundamental properties (ages, masses and extinction values) of the rich star cluster population in the dwarf starburst galaxy NGC 5253. The gain in resolution compared to previous studies is of order a factor of 2 in both spatial dimensions, while our accessible wavelength range transcends previous studies by incorporation of both near-ultraviolet and near-infrared (IR) passbands. We apply spectral synthesis treatments based on two different simple stellar population model suites to our set of medium-, broad-band and H alpha images to gain an improved physical understanding of the IR-excess flux found for a subset of young clusters (30 of 149). With the caveat that our models are based on fully sampled stellar mass functions, the NGC 5253 cluster population is dominated by a significant number of relatively low-mass (M-cl less than or similar to a few x 10(4) M-circle dot) objects with ages ranging from a few x 10(6) to a few x 10(7) yr, which is in excellent agreement with the starburst age of the host galaxy. The IR-excess clusters are almost all found in this young age range and have masses of up to a few x 10(4) M-circle dot. The IR excess in the relatively low-mass NGC 5253 clusters is most likely caused by a combination of stochastic sampling effects and colour variations due to the presence of either luminous red or pre-main-sequence stars. We also find a small number of intermediate-age (similar to 1 Gyr old), similar to 10(5) M-circle dot clusters, as well as up to a dozen massive, similar to 10 Gyr old globular clusters. Their presence supports the notion that NGC 5253 is a very active galaxy that has undergone multiple episodes of star cluster formation.

Place, publisher, year, edition, pages
2013. Vol. 431, no 3, 2917-2932 p.
Keyword [en]
methods: data analysis, stars: luminosity function, mass function, galaxies: starburst, galaxies: star clusters: general, infrared: galaxies
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-90780DOI: 10.1093/mnras/stt392ISI: 000318347500075OAI: oai:DiVA.org:su-90780DiVA: diva2:628644
Funder
Knut and Alice Wallenberg FoundationSwedish Research Council, 2011-5349
Note

AuthorCount:4;

Available from: 2013-06-14 Created: 2013-06-11 Last updated: 2017-12-06Bibliographically approved

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Zackrisson, ErikÖstlin, Göran
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Department of AstronomyThe Oskar Klein Centre for Cosmo Particle Physics (OKC)
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Astronomy, Astrophysics and Cosmology

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