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
    Perspectives on the physics of late-type stars from beyond low earth orbit, the moon and mars
    With the new discoveries enabled thanks to the recent space missions, stellar physics is going through a revolution. However, these discoveries opened the door to many new questions that require more observations. The European Space Agency's Human and Robotic Exploration program provides an excellent opportunity to push forward the limits of our
    Santos, Ângela R. G. et al.

    Fecha de publicación:

    10
    2024
    Bibcode
    2024npjMG..10...96M
    Número de citas
    0
  • Con árbitro
    Echo-free quality factor of a multilayer axion haloscope
    We report a methodology to determine the quality factor ( Q) of wavy dark matter detectors equipped with multilayered resonators, including Fabry-Pérot interferometers and the so-called dielectric haloscope. An anechoic chamber enables the observation of the resonance frequency and its amplitude for an unlimited series of layers for the first time
    DALI Collaboration et al.

    Fecha de publicación:

    10
    2024
    Bibcode
    2024PhRvD.110g2013H
    Número de citas
    0
  • Con árbitro
    Magnetic diffusion in solar atmosphere produces measurable electric fields
    The efficient release of magnetic energy in astrophysical plasmas, such as during solar flares, can in principle be achieved through magnetic diffusion, at a rate determined by the associated electric field. However, attempts at measuring electric fields in the solar atmosphere are scarce, and none exist for sites where the magnetic energy is
    Wöger, Friedrich et al.

    Fecha de publicación:

    10
    2024
    Bibcode
    2024NatCo..15.8811A
    Número de citas
    0