The Temperature of Massive Stars

Bibcode
2004ASSL..315..385G
DOI
10.1007/1-4020-2620-X_78
García, M.; Bianchi, L.
Referencia bibliográfica

How Does the Galaxy Work? A Galactic Tertulia with Don Cox and Ron Reynolds. Edited by Emilio J. Alfaro, Instituto de Astrofica de Andalucía (CSIC), Granada, Spain; Enrique Pérez, Instituto de Astrofíxica de Andalucía (CSIC), Granada, Spain; José Franco, Instituto de Astronomía, UNAM, México. ASTROPHYSICS AND SPACE SCIENCE LIBRARY Volume 315. ISBN 1-4020-2619-6 (HB); ISBN 1-4020-2620-X (e-book). Published by Kluwer Academic Publishers, Dordrecht, The Netherlands, 2004, p.385

Fecha de publicación:
10
2004
Número de autores
2
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Not Available
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    KIC 9163796 - Age determination by asteroseismic grid modelling for an oscillating red giant binary
    The age of a star cannot be measured but only inferred from observational quantities related to age. A wellknown stellar age greatly impacts our understanding of evolution on much larger scales, such as exoplanetary systems or the history of the Milky Way. For stars in the red-giant phase, comparison of observations with evolutionary models
    Grossmann, D. H. et al.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024aecc.conf....7G
    Número de citas
    0
  • Sin árbitro
    Application of Bayesian Inference to disentangle CMB foregrounds
    Both Galactic dust emission and Cosmic infrared background anisotropies (CIB) act as a dominant foreground contaminant for the measurements of the CMB anisotropies (intensity and polarization) at the frequency range above 217 GHz. The Galactic dust and CIB share a similar form of spectral energy distribution, which makes it harder to disentangle
    Adak, Debabrata et al.

    Fecha de publicación:

    1
    2024
    Bibcode
    2024asi..confP..71A
    Número de citas
    0
  • Sin árbitro
    Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems
    The evolution of stars and their hosting binary systems is a highly interactive process and cannot be investigated in a segregated manner. Due to the constraints drawn by stellar binarity, oscillating red-giant stars in binary systems represent a unique opportunity to study the details of the structure and evolution of stars in the advanced phases
    Beck, P. G. et al.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024aecc.conf...24B
    Número de citas
    0