Astrofísicas: Estrellas Wolf-Rayet

  • Publicación
    A spectrophotometric study of the peculiar young open cluster Berkeley 87
    A spectrophotometric study of the peculiar open cluster Berkeley 87 is presented; the measurements show that most of the members are young, heavily reddened OB...
  • Publicación
    Chemical abundances of the WR-ring nebulae NGC 2359 and RCW 78
    This paper reports on extensive spectroscopic observations of the WR-ring nebulae NGC 2359 and RCW 78, respectively, excited by the WN5 stars HD 56925 and WN8...
  • Publicación
    Condensation of dust around the Wolf-Rayet star WR 125
    Infrared photometry of the WC7-type Wolf-Rayet star WR 125 (MR 93) in 1981-91 shows a 10-fold rise in the 3-4 micron flux during 1990-91. This, together with...
  • Noticia
    Descubren la primera explosión de supernova de una estrella Wolf-Rayet
    Un estudio internacional, en el que participan investigadores del Gran Telescopio Canarias (GTC o Grantecan) afiliados al Instituto de Astrofísica de Canarias...
  • Publicación
    Discovery of two new Wolf-Rayet stars from the AAO/UKST H-alpha survey.
    Not Available
  • Publicación
    IRAS 16455-3455 and IRAS 15154-5258 - Two new southern planetary nebulae
    The identification of two new southern planetary nebulae, IRAS 16455-3455 and IRAS 15154-5258, via low resolution spectroscopy, is reported. IRAS 16455-3455 is...
  • Publicación
    On the chemodynamics of Wolf-Rayet ring nebulae - NGC 6888
    Results of a chemodynamical study of the W-R ring nebula NGC 6888 around the WN6 star WR 136 are presented; the observations combine high spatial and spectral...
  • Publicación
    On the O/Fe versus Fe/H relationship and the progenitors of type I supernovae
    The new observational O/Fe versus Fe/H abundance relationship for halo stars is studied in terms of several models of chemical evolution for the solar...
  • Publicación
    On the widths of emission lines in spectra of WC9 stars of different kinds
    Emission lines in the spectra of WC9 stars have been studied. It is shown that there are clear differences between the spectra of BD + 30 3639 and the central...