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Max-Planck-Institut für extraterrestrische Physik


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Papers on Stellar Population models

    1. C. Maraston, 1998, Evolutionary synthesis of stellar populations: a modular tool MNRAS 300, 872-892
    2. C. Maraston, D. Thomas, 2000, Strong Balmer lines in old stellar populations: no need for young ages in ellipticals? ApJ, 541, 126-133
    3. C. Maraston, M. Kissler-Patig, J.P. Brodie, P. Barmby, J.P. Huchra, 2001, The AGB phase-transition outside the local group: K-band observations of young star clusters in NGC 7252 A&A, 370, 176-193
    4. P. Goudfrooij, M. Victoria Alonso, C. Maraston, D. Minniti, 2001, The star cluster system of the 3-Gyr-old merger remnant NGC 1316: clues from optical and near-infrared photometry MNRAS, 328, 237-256
    5. C. Maraston, L. Greggio, A. Renzini, S. Ortolani, R.P. Saglia, T.H. Puzia, M. Kissler-Patig, 2003, Integrated spectroscopy of bulge globular clusters and fields II. Implications for population synthesis models and elliptical galaxies A&A, 400, 823-840
    6. D. Thomas, C. Maraston, 2003, The impact of α/Fe enhanced stellar evolutionary tracks on the ages of elliptical galaxies A&A, 401, 429-432
    7. D. Thomas, C. Maraston, R. Bender, 2003, Stellar population models of Lick indices with variable element abundace ratios MNRAS, 339, 897-911
    8. F.R. Ferraro, L. Origlia, V. Testa, C. Maraston, 2004, Probing the red giant branch phase transition: near-infrared photoemtry of six intermediate-age large magellanic cloud clusters ApJ, 608, 772-780
    9. D. Thomas, C. Maraston, A. Korn, 2004, Higher-order Balmer line indices in α/Fe-enhanced stellar population models MNRAS, 351, L19-L23

last update: 11/2004, editor of this page: Roberto Philip Saglia


 

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