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Chemical and physical properties of nearby population I stars

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Abstract

An analysis of some photometric and kinematic data for nearby Population I stars has been carried out. The main results show that a good correlation exists between the dynamic state and age; but a non-negligible chemical inhomogeneity seems to be present in the disk, independently of the age.

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Authors and Affiliations

  1. Laboratorio di Astrofisica Spaziale, CNR, Frascati, Italy

    D. Cardini & I. Mazzitelli

  2. Laboratorio di Ricerca e Tecnologia per lo studio del Plasma nello Spazio, CNR, Frascati, Italy

    L. Rossi

Authors
  1. D. Cardini
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  2. I. Mazzitelli
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  3. L. Rossi
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Cardini, D., Mazzitelli, I. & Rossi, L. Chemical and physical properties of nearby population I stars. Astrophys Space Sci 48, 283–292 (1977). https://doi.org/10.1007/BF00648116

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  • DOI: https://doi.org/10.1007/BF00648116

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