Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Insights from super-metal-rich stars: Is the Milky Way bar young?
    Context: Bar formation and merger events can contribute to the rearrangement of stars within the Galaxy in addition to triggering star formation (SF) epochs. Super-metal-rich (SMR) stars found in the solar neighbourhood (SNd) can be used as tracers of such events as they are expected to originate only in the inner Galaxy and to have definitely
    Nepal, Samir et al.

    Advertised on:

    7
    2024
    Citations
    0
  • JWST and cross-correlation techniques: A faster alternative for atmospheric studies
    The application of cross-correlation techniques to JWST transmission spectra has opened an alternate pathway to study exoplanet atmospheres with JWST observations, which will contribute to pave the road for the first atmospheric studies with ELTs. JWST observed for the first time the hot-Jupiter WASP-39b on July 2022 as part of the JWST Transiting
    Esparza-borges, Emma et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Localised and transient impact of nuclear activity on the central kiloparsec of galaxies
    Observational and theoretical evidence supports the idea that the influence of supermassive black hole growth on galaxies extends from the central tens of parsecs (localised, transient impact) to hundreds of kiloparsecs (global, long-term impact). Because of the completely different scales of these localised and global effects on the host galaxies
    Ramos Almeida, Cristina

    Advertised on:

    7
    2024
    Citations
    0
  • Magnetic activity of red giants: linking chromospheric indicators, oscillations amplitude, and tidal interactions
    According to dynamo theory, stars with convective envelopes efficiently generate surface magnetic fields, which manifest as magnetic activity in the form of starspots, faculae, and/or flares, when their rotation period is shorter than their convective turnover time. Most red giants, having undergone significant spin down while expanding, have slow
    Gehan, Charlotte et al.

    Advertised on:

    7
    2024
    Citations
    0
  • MARVEL - an array of four telescopes feeding a stabilised spectrograph for high-precision radial velocities of stars
    Mercator Array for Radial VELocities (MARVEL) is an ensemble of four 80-cm off the shelf telescopes feeding a single stabilised high-resolution (R>90 000) echelle spectrograph. The facility is currently under construction and will be located on La Palma (Canary Islands), next to the Mercator telescope. The facility is designed such that the four
    Tkachenko, Andrew et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Mass and radius determination of young planets and the implications for their gas envelope evolution
    Despite thousands of extrasolar planets discovered to date, the dominant mechanisms forming planets and the timescales of planetary migration and atmospheric evaporation remain to be probed observationally. To shed light on these mechanisms, we performed a combined photometric and spectroscopic analysis of several young transiting systems at
    Mallorquín Díaz, Manuel et al.

    Advertised on:

    7
    2024
    Citations
    0