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Discovery of the Galactic Bar Population

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Part of the book series: ESO Astrophysics Symposia ((ESO))

Abstract

The discovery of the Galactic Bar Population is reported from a detailed analysis of the OGLE star counts (Paczyński et al. 1994) in Baaders Window (1°.0, 3°.9). A better agreement between the observed and the simulated star counts is obtained through the introduction of the ‘bar’ population, which has an age in the range 8–9 Gyr and a metallicity between 0.005 < Z < 0.030.

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References

  • Bertelli, G., Bressan, A., Chiosi, C., Ng, Y.K., Ortolani, S., 1995a, A&A 301, 381

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  • Bertelli, G., Bressan, A., Chiosi, C., Ng, Y.K., 1995b, A&A in press

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  • Ng, Y.K., 1995, Ph.D. thesis, Leiden University, the Netherlands

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  • Ng, Y.K., Bertelli, G., Bressan, A., Chiosi, C., Lub, J., 1995a, A&A 295, 655

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  • Ng, Y.K., Bertelli, G., Chiosi, C., Bressan, A., 1995b, A&A submitted

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  • Ng, Y.K., Bertelli, G., Bressan, A., Chiosi, C., 1995c, in preparation

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  • Paczyński, B., Stanek, K.Z., Udalski, A., Szymański, M., Kaluzny, J., Kubiak, M., Mateo, M., 1994, AJ 107, 2060

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© 1996 Springer-Verlag Berlin Heidelberg

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Ng, Y.K., Bertelli, G., Chiosi, C., Bressan, A. (1996). Discovery of the Galactic Bar Population. In: Minniti, D., Rix, HW. (eds) Spiral Galaxies in the Near-IR. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49739-4_15

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  • DOI: https://doi.org/10.1007/978-3-540-49739-4_15

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-662-22429-8

  • Online ISBN: 978-3-540-49739-4

  • eBook Packages: Springer Book Archive

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