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/

  • The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at z {∼} 0
    We report the bivariate $HI$ - and $H 2$ -stellar mass distributions of local galaxies in addition of an inventory of galaxy mass functions, MFs, for $HI$ , $H 2$ , cold gas, and baryonic mass, separately into early- and late-type galaxies. The MFs are determined using the $HI$ and $H 2$ conditional distributions and the galaxy stellar mass
    Rodríguez-Puebla, Aldo et al.

    Advertised on:

    0
    2020
    Citations
    24
  • The age of the Hyades from the lithium depletion boundary.
    The determination of the observational limit below which the cores of very-low mass objects do not reach high enough temperatures and pressure for lithium destruction is called the lithium depletion boundary (LDB). Up to now, the LDB has been used to derive ages of several open clusters younger than 200 Myr, age considered as the practical upper
    Lodieu, N.

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    0
    2020
    Citations
    12
  • The 3D structure of the penumbra at high resolution from the bottom of the photosphere to the middle chromosphere
    Sunspots are the most prominent feature of the solar magnetism in the photosphere. Although they have been widely investigated in the past, their structure remains poorly understood. Indeed, due to limitations in observations and the complexity of the magnetic field estimation at chromospheric heights, the magnetic field structure of sunspot above
    Murabito, Mariarita et al.

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    0
    2020
    Citations
    0
  • Perseus - A Huge Reservoir of Dark Matter investigated with MAGIC
    Galaxy clusters are excellent targets for high energy astrophysics with gamma rays. Not only they may host active galaxies, but they are often expected to provide signatures of accelerations of electrons and protons to PeV energies. Furthermore, according to ΛCDM scenario, they should be embedded in an extremely massive dark matter halo, the
    Doro, Michele et al.

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    0
    2020
    Citations
    0
  • Observations of Li-rich giant stars in the Galaxy and in the Magellanic Clouds
    The Lithium content in stars is very sensitive to the internal stellar conditions. Indeed, Lithium is readily destroyed in the interiors of low-mass main-sequence (MS) stars and the Li in the convective envelope is progressively depleted. The Li abundance at the stellar surface was expected to be further depleted after stars leave the MS and
    García-Hernández, D. A.

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    0
    2020
    Citations
    0
  • Modelling the emission of passive galaxy candidates at z∼3
    Early-type galaxies (ETGs) are of crucial importance to trace back the galaxy mass assembly across cosmic time, yet their formation and quenching remain remarkably elusive. The discoveries of massive, dead galaxies at ever-growing redshifts provided compelling evidence to push their formation up to redshift > 4-5 when the Universe was barely 1 Gyr
    D'Eugenio, C. et al.

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    0
    2020
    Citations
    0