Tipo de publicación: Con árbitro

  • Publicación
    Mass Production of 2023 KMTNet Microlensing Planets. II. Two Planets and A Brown Dwarf
    To expand the homogeneous microlensing planetary sample of the Korea Microlensing Telescope Network (KMTNet), we investigate six planetary candidates identified...
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    Mass Ratio Determination from H α Lines in Black Hole X-Ray Transients
    We find that the mass ratio q in quiescent black hole (BH) X-ray transients is tightly correlated with the ratio of the double-peak separation (DP) to the full...
  • Publicación
    Mass ratio from Doppler beaming and Rømer delay versus ellipsoidal modulation in the Kepler data of KOI-74
    We present a light-curve analysis and radial velocity study of KOI-74, an eclipsing A star + white dwarf binary with a 5.2-d orbit. Aside from new spectroscopy...
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    Mass spectrometric analysis of selected radiolyzed amino acids in an astrochemical context
    A selection of amino acids, namely arginine, proline and tyrosine previously irradiated to 3.2 mega-Gray in the solid state and analyzed by differential...
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    Mass-loss of globular cluster red giants - A semi-empirical estimation
    Limits to the total mass-loss in red giants in globular clusters are calculated on the basis of Sweigart and Gross (1976) Horizontal Branch models by means of...
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    Mass-metallicity relation explored with CALIFA. I. Is there a dependence on the star-formation rate?
    We studied the global and local M-Z relation based on the first data available from the CALIFA survey (150 galaxies). This survey provides integral field...
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    Mass-metallicity relation of dwarf galaxies and its dependency on time: clues from resolved systems and comparison with massive galaxies
    Aims: We present a new approach to study the mass-metallicity relation and its dependency on time. Methods: We used the star formation history (SFH) derived...
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    Mass-to-light ratios from the fundamental plane of spiral galaxy discs
    The best-fitting two-dimensional plane within the three-dimensional space of spiral galaxy disc observables (rotational velocity vrot, central disc surface...
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    Masses and ages for metal-poor stars. A pilot programme combining asteroseismology and high-resolution spectroscopic follow-up of RAVE halo stars
    Context. Very metal-poor halo stars are the best candidates for being among the oldest objects in our Galaxy. Samples of halo stars with age determination and...