Constraints to the mass loss rate of globular cluster red giants

Bibcode
1990A&A...231...95P
Paez, E.; Martinez Roger, C.; Manteiga, M.; Arribas, S.
Referencia bibliográfica

Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 1, May 1990, p. 95-99.

Fecha de publicación:
5
1990
Número de autores
4
Número de autores del IAC
4
Número de citas
1
Número de citas referidas
1
Descripción
The expected mass loss rates from horizontal branch (HB) and red giant branch models are investigated. The expected dependence of those rates on luminosity, metallicity, helium content, giant mass, and HB morphology is discussed. For an HB distribution depending on metallicity, the values found for the fitting factors in the Reimers parameterization are in good agreement with those derived independently for Population I stars.
Tipo
Con árbitro
Estrellas gigantes rojas

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