Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • The VLT-FLAMES Tarantula Survey
    The VLT-FLAMES Tarantula Survey (VFTS) was an ESO Large Programme that has provided a rich, legacy dataset for studies of both resolved and integrated populations of massive stars. Initiated in 2008 (ESO Period 82), we used the Fibre Large Array Multi Element Spectrograph (FLAMES) to observe more than 800 massive stars in the dramatic 30 Doradus
    Evans, C. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    5
  • The T<SUB>e</SUB>[N II]-T<SUB>e</SUB>[O III] temperature relation in H II regions and the reliability of strong-line methods
    We use a sample of 154 observations of 124 H II regions that have measurements of both T e[O III] and T e[N II], compiled from the literature, to explore the behaviour of the T e[O III]-T e[N II] temperature relation. We confirm that the relation depends on the degree of ionization and present a new set of relations for two different ranges of this
    Arellano-Córdova, K. Z. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    32
  • The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
    We present the final Sloan Digital Sky Survey IV (SDSS-IV) quasar catalog from Data Release 16 of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). This catalog comprises the largest selection of spectroscopically confirmed quasars to date. The full catalog includes two subcatalogs (the current versions are DR16Q_v4 and DR16Q_Superset
    Lyke, Brad W. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    422
  • The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136
    We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of the Large Magellanic Cloud. Our sample was observed with STIS aboard the Hubble Space Telescope, is complete down to about 40 M ☉, and includes seven very massive stars with masses over 100 M ☉. We performed a spectroscopic analysis to derive their
    Bestenlehner, Joachim M. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    80
  • The post-common-envelope binary central star of the planetary nebula ETHOS 1
    We present a detailed study of the binary central star of the planetary nebula ETHOS 1 (PN G068.1+11.0). Simultaneous modelling of light and radial velocity curves reveals the binary to comprise a hot and massive pre-white dwarf with an M-type main-sequence companion. A good fit to the observations was found with a companion that follows expected
    Munday, James et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    14
  • The participation of the IAC in the ESA-SSA P3NEOI program.
    Introduction: The Solar System group of the Instituto de Astrofisica de Canarias (IAC) is member of a consortium of astronomical observatories leaded by Deimos Space S.L.U, that presented a proposal to the ESA ITT no. AO/1-9591/18/D/MR "P3-NEO-I - Observational support from collaborating observatories". The objective of this project is to provide
    Licandro, Javier et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    1