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  1. Home
  2. Browse by Author

Browsing by Author "Goudfrooij, P."

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    Compact stellar systems in the polar ring galaxies NGC4650A and NGC3808B : Clues to polar disk formation
    (2016) Ordenes Briceño, Y.; Georgiev, I.; Puzia, Thomas H.; Goudfrooij, P.; Arnaboldi, M.
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    Extended Main Sequence Turnoffs in Intermediate-Age Star Clusters : A Correlation Between Turnoff Width and Early Escape Velocity
    (2014) Goudfrooij, P.; Girardi, L.; Kozhurina-Platais, V.; Kalirai, J.; Platais, I.; Puzia, Thomas H.; Correnti, M.; Bressan, A.; Chandar, R.
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    Extragalactic globular clusters in the near infrared - III. NGC 5846 and NGC 7192 - Quantifying the age distribution of sub-populations
    (2003) Hempel, M.; Hilker, M.; Kissler-Patig, M.; Puzia, T.H.; Minniti, D.; Goudfrooij, P.
    In this third paper of our series on near-IR and optical photometry of globular cluster systems in early-type galaxies we concentrate on the photometric results for NGC 5846 and NGC 7192, two group ellipticals, and on a first comparison between the globular cluster systems investigated so far. In NGC 5846 the colour-colour diagram shows clear bi-modality in (V - K), which is confirmed by a KMM test. The mean colour of both peaks were estimated to be (V - K)(blue) = 2.57 +/- 0.06 and (V - K)(red) = 3.18 +/- 0.06. The situation in NGC 7192 is different, in that the colour-colour diagram gives no evidence for a distinct second population of globular clusters. Using simulated colour distributions of globular cluster systems, we make a first step in quantifying the cumulative age distribution in globular cluster systems. Also here the result for NGC 5846 leads us to the conclusion that its metal-rich globular cluster population contains two globular cluster populations which differ in age by several Gyr. The age structure for NGC 7192 shows instead strong similarity with a single-age population.
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    Faint dwarf galaxies in Hickson Compact Group 90
    (2016) Ordenes, Y.; Taylor, M.; Puzia, Thomas H.; Muñoz Soria, Roberto; Eigenthaler, P.; Georgiev, I.; Goudfrooij, P.; Hilker, M.; Lancon, A.; Mamon, G.; Mieske, S.; Miller, B.; Peng, E.; Sanchez, R.
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    Hubble Space Telescope Observations of Globular Cluster Systems Along the Hubble Sequence of Spiral Galaxies
    (2003) Goudfrooij, P.; Minniti, D.
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    Kinematics, ages and metallicities of star clusters in NGC 1316: a 3-Gyr-old merger remnant
    (2001) Goudfrooij, P.; Minniti, D.
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    Luminosity function of low-mass X-ray binaries in the globular cluster system of NGC 1399
    (2014) D’Ago, Giuseppe; Paolillo, M.; Fabbiano, G.; Puzia, Thomas H.; Maccarone, T.J.; Kundu, A.; Goudfrooij, P.; Zepf, S.E.
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    New constraints on the star formation history of the star cluster NGC 1856
    (2015) Correnti, M.; Goudfrooij, P.; Puzia, Thomas H.; De Mink, S.
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    On the interpretation of sub-giant branch morphologies of intermediate-age star clusters with extended main sequence turnoffs
    (2015) Goudfrooij, P.; Girardi, L.; Rosenfield, P.; Bressan, A.; Marigo, P.; Correnti, M.; Puzia, Thomas H.
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    Population parameters of intermediate-age star clusters in the Large Magellanic Cloud, I. NGC 1846 and its wide main sequence turnoff
    (2009) Goudfrooij, P.; Puzia, Thomas H.
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    Population Parameters of Intermediate-age Star Clusters in the Large Magellanic Cloud. II. New Insights from Extended Main-sequence Turnoffs in Seven Star Clusters
    (2011) Goudfrooij, P.; Puzia, Thomas H.
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    Population Parameters of Intermediate-age Star Clusters in the Large Magellanic Cloud. III. Dynamical Evidence for a Range of Ages Being Responsible for Extended Main-sequence Turnoffs
    (2011) Goudfrooij, P.; Puzia, Thomas H.
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    The Star Cluster System of the 3-Gyr-Old Merger Remnant NGC 1316: Clues From Optical and Near-Infrared Photometry
    (2001) Goudfrooij, P.; Minniti, D.
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    The Strikingly Metal-rich Halo of the Sombrero Galaxy
    (2020) Cohen, R. E.; Goudfrooij, P.; Correnti, M.; Gnedin, O. Y.; Harris, W. E.; Chandar, R.; Puzia, Thomas H.; Sánchez Janssen, R.

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