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/

  • Refereed
    Characterization of the June epsilon Ophiuchids meteoroid stream and the comet 300P/Catalina
    Aims: Prior to 2019, the June epsilon Ophiuchids (JEO) were known as a minor unconfirmed meteor shower with activity that was considered typically moderate for bright fireballs. An unexpected bout of enhanced activity was observed in June 2019, which even raised the possibility that it was linked to the impact of the small asteroid 2019 MO near
    Matlovič, Pavol et al.

    Advertised on:

    4
    2020
    Bibcode
    2020A&A...636A.122M
    Citations
    11
  • Refereed
    Characterization of M-stars in the LMC in the JWST era
    We study the M-type asymptotic giant branch (AGB) population of the Large Magellanic Cloud (LMC) by characterizing the individual sources in terms of the main properties of the progenitors and of the dust present in the circumstellar envelope. To this aim we compare the combination of the spectroscopic and photometric data collected by Spitzer
    Marini, E. et al.

    Advertised on:

    4
    2020
    Bibcode
    2020MNRAS.493.2996M
    Citations
    10
  • Thesis
    CARACTERIZACIÓN ESPECTRAL DE LA SUPERFICIE DEL ASTEROIDE (101955) BENNU A TRAVÉS DEL CONJUNTO INSTRUMENTAL OCAMS DE LA SONDA OSIRIS-REX
    Los asteroides son objetos resultantes de las colisiones y evolución dinámica de los planetesimales originarios del Sistema Solar. Algunos de estos planetesimales originarios —formados en el disco protoplanetario como consecuencia de la agregación de gas y polvo— sobrevivieron al proceso de formación planetaria y permanecen prácticamente
    Juan Luis Rizos García

    Advertised on:

    4
    2020
    Bibcode
    TESIS
  • Thesis
    CARACTERIZACIÓN ESPECTRAL DE LA SUPERFICIE DEL ASTEROIDE (101955) BENNU A TRAVÉS DEL CONJUNTO INSTRUMENTAL OCAMS DE LA SONDA OSIRIS-REX
    Los asteroides son objetos resultantes de las colisiones y evolución dinámica de los planetesimales originarios del Sistema Solar. Algunos de estos planetesimales originarios —formados en el disco protoplanetario como consecuencia de la agregación de gas y polvo— sobrevivieron al proceso de formación planetaria y permanecen prácticamente
    Juan Luis Rizos García

    Advertised on:

    4
    2020
    Bibcode
    Link
  • Refereed
    Candidate LBV stars in galaxy NGC 7793 found via HST photometry + MUSE spectroscopy
    Only about 19 Galactic and 25 extragalactic bonafide luminous blue variables (LBVs) are known to date. This incomplete census prevents our understanding of this crucial phase of massive star evolution which leads to the formation of heavy binary black holes via the classical channel. With large samples of LBVs one could better determine the
    Wofford, Aida et al.

    Advertised on:

    4
    2020
    Bibcode
    2020MNRAS.493.2410W
    Citations
    12
  • Refereed
    Candidate Brown-dwarf Microlensing Events with Very Short Timescales and Small Angular Einstein Radii
    Short-timescale microlensing events are likely to be produced by substellar brown dwarfs (BDs), but it is difficult to securely identify BD lenses based on only event timescales t E because short-timescale events can also be produced by stellar lenses with high relative lens-source proper motions. In this paper, we report three strong candidate BD
    Han, Cheongho et al.

    Advertised on:

    4
    2020
    Bibcode
    2020AJ....159..134H
    Citations
    16