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/

  • Galaxy size trends as a consequence of cosmology
    We show that recently documented trends in galaxy sizes with mass and redshift can be understood in terms of the influence of underlying cosmic evolution; a holistic view which is complimentary to interpretations involving the accumulation of discreet evolutionary processes acting on individual objects. Using standard cosmology theory, supported
    Stringer, M. J. et al.

    Advertised on:

    6
    2014
    Citations
    21
  • FORMATION AND EVOLUTION OF EARLY-TYPE DWARF GALAXIES: A TWO-DIMENSIONAL PERSPECTIVE
    AGNIEZKA RYS

    Advertised on:

    6
    2014
  • First Results from HST19 GO12600: CNO Abundances in Seven Milky Way Planetary Nebulae
    In HST Cycle 19 we observed 10 Milky Way planetary nebulae (PNe) from 1150-10270Å with STIS to obtain accurate abundances of carbon, nitrogen and oxygen. The ultimate goal of the project is to assess carbon production in the low-to-intermediate-mass (LIMS) progenitors of PNe with near-solar metallicity 0.5-1.2 x solar), but varying N/O 0.1-3)
    Kwitter, K. B. et al.

    Advertised on:

    6
    2014
    Citations
    0
  • Depolarizing Collisions with Hydrogen: Neutral and Singly Ionized Alkaline Earths
    Depolarizing collisions are elastic or quasielastic collisions that equalize the populations and destroy the coherence between the magnetic sublevels of atomic levels. In astrophysical plasmas, the main depolarizing collider is neutral hydrogen. We consider depolarizing rates on the lowest levels of neutral and singly ionized alkali earths Mg I, Sr
    Manso Sainz, R. et al.

    Advertised on:

    6
    2014
    Citations
    16
  • Chemical abundances of stars with brown-dwarf companions
    Context. It is well known that stars with giant planets are, on average, more metal-rich than stars without giant planets, whereas stars with detected low-mass planets do not require to be metal-rich. Aims: With the aim of studying the weak boundary that separates giant planets and brown dwarfs (BDs) and their formation mechanism, we analyze the
    Mata Sánchez, D. et al.

    Advertised on:

    6
    2014
    Citations
    12
  • Beam asymmetry Σ in η' photoproduction off the proton at the GRAAL experiment
    The only recent η' photoproduction data off proton available in literature are the differential and total cross sections published by the CLAS and CB-ELSA-TAPS Collaborations. However, the wide information about reaction cross sections are not sufficient to understand the role of resonances involved in the process. Different theoretical works
    Mandaglio, G. et al.

    Advertised on:

    6
    2014
    Citations
    0