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..

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  • The eccentricity distribution of warm sub-Saturns in TESS
    We present the eccentricity distribution of warm sub-Saturns (4–8 $R_{\rm{\oplus }}$, 8–200 d periods) as derived from an analysis of transit light curves from NASA's Transiting Exoplanet Survey Satellite (TESS) mission. We use the 'photoeccentric' effect to constrain the eccentricities of 76 planets, comprising 60 and 16 from single and
    Fairnington, Tyler R. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • V4141 Sgr: Outflows and repeated outbursts
    In this work, we analyze the ongoing brightening of the poorly studied symbiotic star V4141 Sgr and examine its long-term variability. We present new low-resolution spectroscopic observations of the system in its bright state and combine them with multi-color photometric data from our observations, as well as ASAS-SN, ATLAS, and Gaia DR3. To
    Merc, Jaroslav et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • ASASSN–14dx: a cataclysmic variable harbouring a massive pulsating white dwarf
    We present the results of our study of ASASSN–14dx, a previously known but poorly characterized cataclysmic variable (CV). The source was observed as part of an ongoing high-time-resolution photometric survey of CVs, which revealed that, in addition to the known 82.8-min orbital period, it also exhibits other transient periods, the strongest of
    Hakala, Pasi et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at Z = 0.2 Z<SUB>⊙</SUB>
    Early B-type stars with initial masses between 8 and 15 M ⊙ are frequently found in multiple systems, as is evidenced by multi-epoch spectroscopic campaigns in the Milky Way and the Large Magellanic Cloud (LMC). Previous studies have shown no strong metallicity dependence in the close-binary (a < 10 au) fraction or orbital-period distributions
    Villaseñor, J. I. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    4
  • The properties of the obscuring material of a sample of active galactic nuclei from mid-IR and X-ray simultaneous fitting
    Context. Over ten mid-infrared (mid-IR) and X-ray models are currently attempting to describe the nuclear obscuring material of active galactic nuclei (AGNs), but many questions remain unresolved. Aims. This study aims to determine the physical parameters of the obscuring material in nearby AGNs and explore their relationship with nuclear activity
    Esparza-Arredondo, D. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey
    The Wide Angle Search for Planets (WASP) survey provided some of the first transiting hot Jupiter candidates. With the addition of the Transiting Exoplanet Survey Satellite (TESS), many WASP planet candidates have now been revisited and given updated transit parameters. Here, we present nine transiting planets orbiting FGK stars that were
    Schanche, N. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0