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

  • Con árbitro
    The XMM-Newton/HST View of the Obscuring Outflow in the Seyfert Galaxy Mrk 335 Observed at Extremely Low X-Ray Flux
    The Seyfert galaxy Mrk 335 is known for its frequent changes of flux and spectral shape in the X-ray band that occurred during recent years. These variations may be explained by the onset of a wind that previous, noncontemporaneous high-resolution spectroscopy in X-ray and UV bands located at accretion disk scale. A simultaneous new campaign by XMM
    Longinotti, Anna Lia et al.

    Fecha de publicación:

    4
    2019
    Bibcode
    2019ApJ...875..150L
    Número de citas
    40
  • Con árbitro
    The VLT-FLAMES Tarantula Survey. XXXI. Radial velocities and multiplicity constraints of red supergiant stars in 30 Doradus
    Aims: The incidence of multiplicity in cool, luminous massive stars is relatively unknown compared to their hotter counterparts. In this work we present radial velocity (RV) measurements and investigate the multiplicity properties of red supergiants (RSGs) in the 30 Doradus region of the Large Magellanic Cloud using multi-epoch visible spectroscopy
    Patrick, L. R. et al.

    Fecha de publicación:

    4
    2019
    Bibcode
    2019A&A...624A.129P
    Número de citas
    33
  • Con árbitro
    The VLT-FLAMES Tarantula Survey. XXX. Red stragglers in the clusters Hodge 301 and SL 639
    Aims: We estimate physical parameters for the late-type massive stars observed as part of the VLT-FLAMES Tarantula Survey (VFTS) in the 30 Doradus region of the Large Magellanic Cloud (LMC). Methods: The observational sample comprises 20 candidate red supergiants (RSGs) which are the reddest ((B - V) > 1 mag) and brightest (V 16 mag) objects in
    Britavskiy, N. et al.

    Fecha de publicación:

    4
    2019
    Bibcode
    2019A&A...624A.128B
    Número de citas
    44
  • Con árbitro
    The Type II-plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor
    We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 2017eaw is a normal SN II-P intermediate in properties between, for example, SN 1999em and SN 2012aw and the more luminous SN 2004et, also in NGC 6946. We have determined
    Van Dyk, Schuyler D. et al.

    Fecha de publicación:

    4
    2019
    Bibcode
    2019ApJ...875..136V
    Número de citas
    81
  • Con árbitro
    The MUSE Atlas of Disks (MAD): resolving star formation rates and gas metallicities on <100 pc scales†
    We study the physical properties of the ionized gas in local discs using the sample of 38 nearby ˜108.5-11.2 M⊙ Star-Forming Main-Sequence (SFMS) galaxies observed so far as part of the MUSE Atlas of Disks (MAD). Specifically, we use all strong emission lines in the MUSE wavelength range 4650-9300 Å to investigate the resolved ionized gas
    Erroz-Ferrer, Santiago et al.

    Fecha de publicación:

    4
    2019
    Bibcode
    2019MNRAS.484.5009E
    Número de citas
    107
  • Sin árbitro
    The Evolutionary history of the Milky Way discs and halo from Gaia DR2 colour-magnitude diagram fitting
    The technique of color-magnitude diagram (CMD) fitting is a well recognized method that has been used for over 20 years to determine detailed star formation histories (SFH) for Local Group galaxies (Gallart et al. 2005; Tolstoy et al. 2009). The accurate distances for large stellar samples provided in Gaia DR2, together with the precise
    Gallart, Carme et al.

    Fecha de publicación:

    4
    2019
    Bibcode
    2019gaia.confE..40G
    Número de citas
    1