Infrared light curves of the Algol system UX HER

Bibcode
1996ASPC..109..655M
Martinez-Pais, I. G.; Arevalo, M. J.; Lázaro, C.; Antonopoulou, E.; Ferentinios, E.
Referencia bibliográfica

Cool stars; stellar systems; and the sun : 9 : Astronomical Society of the Pacific Conference Series, volume 109; Proceedings of the 9th Cambridge workshop; held 3-6 October 1995 in Florence; Italy; San Francisco: Astronomical Society of the Pacific (ASP); |c1996; edited by Roberto Pallavicini and Andrea K. Dupree, p.655

Advertised on:
0
1996
Número de autores
5
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
    Understanding the thermal and magnetic properties of an X-class flare in the low solar atmosphere
    Recently, the exploitation of spectropolarimetric data has allowed to improve our knowledge of the dynamical and magnetic response of the photospheric and chromospheric layers to the rapid release of energy occurring during solar flares. In this framework, we have used high-resolution observations acquired on 22nd October 2014 during an X1.6
    Ferrente, Fabiana et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..538F
    Número de citas
    0
  • Sin árbitro
    GLACE survey: a window on the evolution of galaxies within clusters. Revealing galaxy evolution within Zw Cl0024.0+1652
    The GLACE (GaLAxy Cluster Evolution) survey represents a groundbreaking effort to explore the evolution of galaxies within galaxy clusters. Using data from the Gran Telescopio de Canarias (GTC), GLACE investigates emission line galaxies (ELGs) and active galactic nuclei (AGN) hosts across various redshifts. Recent observations within the ZwCl 0024
    De Daniloff, Simon B. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.2224D
    Número de citas
    0
  • Sin árbitro
    Accretion-induced variability of interacting red giant binaries masquerading as oscillations
    Symbiotic stars are strongly interacting binaries with long orbital periods, containing an evolved red giant and a white dwarf or a neutron star embedded in a circumbinary nebula. They constitute unique astrophysical laboratories important for understanding the binary evolution and diverse processes occurring also in many other types of
    Merc, Jaroslav et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..966M
    Número de citas
    0