La Vía Láctea y el Grupo Local (MWLG)
  • Publicación
    H α morphologies of star clusters: a LEGUS study of H II region evolution time-scales and stochasticity in low-mass clusters
    The morphology of H II regions around young star clusters provides insight into the time-scales and physical processes that clear a cluster's natal gas. We...
  • Publicación
    H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia
    We present an elemental abundance analysis of high-resolution spectra for five giant stars spatially located within the innermost regions of the bulge globular...
  • Subvención
    Hacia la comprensión de los últimos estados de la evolución estelar y la formación de moléculas orgánicas complejas
    La mayoría de las estrellas (M < 8 masas solares, Ms) terminan sus vidas con una intensa pérdida de masa en la Rama Asintótica de las Gigantes (AGB), justo...
  • Publicación
    Hayabusa2 extended mission target asteroid 1998 KY<SUB>26</SUB> is smaller and rotating faster than previously known
    Understanding the physical characteristics of small Solar System bodies is important not only for refining formation and evolution models but also for space...
  • Publicación
    HD 110067 c has an aligned orbit. Measuring the Rossiter-McLaughlin effect inside a resonant multi-planet system with ESPRESSO
    Planetary systems in mean motion resonances hold a special place among the planetary population. They allow us to study planet formation in great detail as...
  • Publicación
    HD 20329b: An ultra-short-period planet around a solar-type star found by TESS
    Context. Ultra-short-period (USP) planets are defined as planets with orbital periods shorter than one day. This type of planets is rare, highly irradiated, and...
  • Publicación
    Heavy Element Nucleosynthesis in the Brightest Galactic Asymptotic Giant Branch Stars
    We present updated calculations of stellar evolutionary sequences and detailed nucleosynthesis predictions for the brightest asymptotic giant branch (AGB) stars...
  • Publicación
    Heavy-element Abundances in P-rich Stars: A New Site for the s-process?
    The recently discovered phosphorus-rich stars pose a challenge to stellar evolution and nucleosynthesis theory, as none of the existing models can explain their...
  • Publicación
    Heavy-element yields and abundances of asymptotic giant branch models with a Small Magellanic Cloud metallicity
    We present new theoretical stellar yields and surface abundances for asymptotic giant branch (AGB) models with a metallicity appropriate for stars in the Small...