Publicaciones

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  • Multi-year characterisation of the broad-band emission from the intermittent extreme BL Lac 1ES 2344+514
    Aims: The BL Lac 1ES 2344+514 is known for temporary extreme properties characterised by a shift of the synchrotron spectral energy distribution (SED) peak energy ν synch, p above 1 keV. While those extreme states have only been observed during high flux levels thus far, additional multi-year observing campaigns are required to achieve a coherent
    MAGIC Collaboration et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    6
  • More fundamental than the fundamental metallicity relation. The effect of the stellar metallicity on the gas-phase mass-metallicity and gravitational potential-metallicity relations
    Context One of the most fundamental scaling relations in galaxies is observed between metallicity and stellar mass - the mass-metallicity relation (MZR) - although recently a stronger dependence of the gas-phase metallicity with the galactic gravitational potential (ΦZR) has been reported. Further dependences of metallicity on other galaxy
    Sánchez-Menguiano, Laura et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    5
  • Modeling Close Binary Systems Within Planetary Nebulae
    We present here binary modeling for the close binary central star of the planetary nebula Hf 2-2. While binary models for 26 close binary star systems within a planetary nebula exist, this number is far too low to perform a significant statistical analysis. In order to work towards increasing this number, and thus improving the statistical results
    Blanton, Lilly et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    0
  • Modeling Binary Systems Containing the Hot White Dwarfs WD1136+667 and Gaia-DR2-1350
    In this study, we look specifically at binary white dwarfs where the companion is a main sequence star. In particular, we look at very hot white dwarfs, many of which demonstrate the "hydrogen problem" in which modeling of their hydrogen absorption features, and optical features in general, do not appear to give accurate temperatures. The two
    Wood, Hunter et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    0
  • MANCHA3D Code: Multipurpose Advanced Nonideal MHD Code for High-Resolution Simulations in Astrophysics
    The MANCHA3D code is a versatile tool for numerical simulations of magnetohydrodynamic (MHD) processes in solar/stellar atmospheres. The code includes nonideal physics derived from plasma partial ionization, a realistic equation of state and radiative transfer, which allows performing high-quality realistic simulations of magnetoconvection, as well
    Modestov, M. et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    13
  • JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs
    We present JWST images of the well-known planetary nebula NGC 6720 (the Ring Nebula), covering wavelengths from 1.6 to 25 $\, \mu$m. The bright shell is strongly fragmented with some 20 000 dense globules, bright in H 2, with a characteristic diameter of 0.2 arcsec and density n H ~ 10 5-10 6 cm -3. The shell contains a narrow ring of polycyclic
    Wesson, R. et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    17