Tipo de publicación: Con árbitro

  • Publicación
    Minutes-duration optical flares with supernova luminosities
    In recent years, certain luminous extragalactic optical transients have been observed to last only a few days 1. Their short observed duration implies a...
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    Mirach's Goblin: Discovery of a dwarf spheroidal galaxy behind the Andromeda galaxy
    Context. It is of broad interest for galaxy formation theory to carry out a full inventory of the numbers and properties of dwarf galaxies, both satellite and...
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    MIRACLE: I. Unveiling the multi-phase, multi-scale physical properties of the active galaxy NGC 424 with MIRI, MUSE, and ALMA
    We present an analysis of the multi-phase gas properties in the Seyfert II galaxy NGC 424, using spatially resolved spectroscopic data from JWST/MIRI, part of...
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    MIRACLE: II. Unveiling the multiphase gas interplay in the circumnuclear region of NGC 1365 via multicloud modeling
    We present a multiphase analysis of the gas in the circumnuclear region (∼0.9 × 0.9 kpc 2) of the nearby barred Seyfert 1.8 galaxy NGC 1365, observed as part of...
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    Misaligned spin-orbit in the XO-3 planetary system?
    The transiting extrasolar planet XO-3b is remarkable, with a high mass and eccentric orbit. These unusual characteristics make it interesting to test whether...
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    Misleading variations in estimated rotational frequency splittings of solar p modes: consequences for helioseismology and asteroseismology
    The aim of this paper is to investigate whether there are any 11-yr or quasi-biennial solar-cycle-related variations in solar rotational splitting frequencies...
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    Missing dust of super-early galaxies: Supernova blowout and gas─dust venting in blue monsters
    Context. A subset of very young super-early galaxies at z ≳ 10, often called blue monsters, shows extremely blue UV continua and faint far-IR emission. This...
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    Missing large-angle correlations versus even-odd point-parity imbalance in the cosmic microwave background
    Context. The existence of a maximum correlation angle (θ max ≳ 60°) in the two-point angular temperature correlations of cosmic microwave background (CMB)...
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    MIUSCAT: extended MILES spectral coverage - I. Stellar population synthesis models
    We extend the spectral range of our stellar population synthesis models based on the MILES and CaT empirical stellar spectral libraries. For this purpose, we...