Tipo de publicación: Con árbitro

  • Publicación
    The distribution of galaxy morphological types and the morphology-mass relation in different environments at low redshift
    We use ˜2000 galaxies from PM2GC (Calvi, Poggianti & Vulcani 2011a) belonging to different environments to show how the fractions of different galaxy...
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    The Distribution of Quiet Sun Magnetic Field Strengths from 0 to 1800 G
    The quiet-Sun photospheric plasma has a variety of magnetic field strengths going from zero to 1800 G. The empirical characterization of these field strengths...
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    The distribution of sunspot decay rates
    The distribution of sunspot decay rates is studied using the Greenwich Photoheliographic Results (GPR) for a total of approximately hundred years between 1874...
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    The distribution of the local interstellar medium derived from MG II column densities towards seven cool stars
    High resolution spectra containing the Mg II h and k resonance doublet have been obtained using the long wavelength spectrometer of IUE, for 7 late-type stars...
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    The diverse cold molecular gas contents, morphologies, and kinematics of type-2 quasars as seen by ALMA
    We present CO(2−1) and adjacent continuum observations of seven nearby radio-quiet type-2 quasars (QSO2s) obtained with ALMA at ∼0.2″ resolution (370 pc at z ∼...
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    The diverse density profiles of galaxy clusters with self-interacting dark matter plus baryons
    We present the first simulated galaxy clusters (M200 > 1014 M⊙) with both self-interacting dark matter (SIDM) and baryonic physics. They exhibit a greater...
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    The dolmens and "Hawanat" of Africa Proconsularis revisited
    Not Available
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    The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1
    Aims: The role of galaxy mergers in massive galaxy evolution, and in particular to mass assembly and size growth, remains an open question. In this paper we...
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    The donor of Aquila X-1 revealed by high-angular resolution near-infrared spectroscopy
    The low-mass X-ray binary Aquila X-1 is one of the most active neutron star X-ray transients. Despite its relatively bright quiescent optical counterpart, the...