Esta web estará fuera de servicio por mantenimiento el lunes 6 de mayo de 7:30 a 8:00.

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

Te puede interesar

  • Con árbitro
    High-resolution Spectroscopic Reconnaissance of a Temperate Sub-Neptune
    The study of temperate sub-Neptunes is the new frontier in exoplanetary science. A major development in the past year has been the first detection of carbon-bearing molecules in the atmosphere of a temperate sub-Neptune, K2-18 b, a possible Hycean world, with the James Webb Space Telescope (JWST). The JWST is poised to characterize the atmospheres
    Cabot, Samuel H. C. et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024ApJ...966L..10C
    Número de citas
    0
  • Con árbitro
    Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST
    JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5000 confirmed planets, more than 4000 Transiting Exoplanet Survey Satellite (TESS) planet candidates are still unconfirmed and many of the best planets for atmospheric characterization may remain to be identified. We present a sample
    Hord, Benjamin J. et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024AJ....167..233H
    Número de citas
    0
  • Con árbitro
    Nonlinear Wave Damping by Kelvin–Helmholtz Instability-induced Turbulence
    Magnetohydrodynamic kink waves naturally form as a consequence of perturbations to a structured medium, for example, transverse oscillations of coronal loops. Linear theory has provided many insights into the evolution of linear oscillations, and results from these models are often applied to infer information about the solar corona from observed
    Hillier, Andrew et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024ApJ...966...68H
    Número de citas
    0