Publication type: Non-refereed

  • Publication
    Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations
    We present FIES@NOT and HARPS-N@TNG radial velocity follow-up observations of K2-19, a compact planetary system hosting three planets, of which the two larger...
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    Mass distributions in disk galaxies
    We present results on luminous and dark matter mass distributions in disk galaxies from the DiskMass Survey. As expected for normal disk galaxies, stars...
  • Publication
    Mass function of IC4665 from UKIDSS-GCS (Lodieu+, 2011)
    Knowledge of the mass function in open clusters constitutes one way to constrain the formation of low-mass stars and brown dwarfs along with the knowledge of...
  • Publication
    Mass loss from an extreme OH/IR star: OH 26.5+0.6
    Observations of H2O isotopologues of the extreme OH/IR star OH 26.5+0.6 show that the star has an initial mass consistent with it being an intermediate-mass...
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    Mass Loss in Galactic Globulars: Red Giant Stragglers and Helium White Dwarfs
    The evolution of Population II Red Giants has been studied by adopting Reimers' formalism for the efficiency of mass loss. Evolutionary computations for models...
  • Publication
    Mass, metallicity and SFR relationships in star forming galaxies using deep surveys
    Not Available
  • Publication
    Massive AGB Stars in the Early Solar System?
    We present evidence that recently identified massive rubidium-rich AGB stars also played an important role as sources of certain long-lived and short-lived...
  • Publication
    Massive characterisation of subgiants and red giants with TESS (Kepler and Gaia)
    TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as...
  • Publication
    Massive compact galaxies in the local Universe: what are they?
    Recent investigations have provided evidences that many massive (M_* > 10^{11} M_&sun;) spheroid galaxies in the early universe (z ≥ 1.5) were extremely compact...