Tipo de publicación: Sin árbitro

  • Publicación
    Detection of large terrestrial planets around M and K dwarf stars in Orion by transit photometry
    A ground based transit survey of M and K-dwarf stars near the galactic plane should be able to determine the abundance of the lower end of the planetary radius...
  • Publicación
    Detection of lithium in massive stars
    Lithium in stars more massive than ∼6 M ☉ is expected to be totally depleted by the time when the stars reach the He core burning phase, as a consequence of...
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    Detection of narrow C 4 and SI 4 absorption features in spectra of stars within 200 PC F the Sun
    Detection of narrow (δλ 0.5 Å) absorption features in C IV at λλ1548 and 1550 have been made in the spectra of 4 late B dwarfs within 200 pc of the sun; the Si...
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    Detection of Neodymium in APOGEE H-band Spectra and its Application to Chemical Tagging
    We report the successful detection of the rare earth element Neodymium (Nd) in the high-resolution, H-band spectra from the SDSS III Apache Point Observatory...
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    Detection of New Planetary Nebulae by IPHAS, the Hα Survey of the North Galactic Plane
    IPHAS is an ongoing Hα imaging survey of the North Galactic plane. When completed, it is expected to discover several hundred new Galactic planetary nebulae, in...
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    Detection of periodic signatures in the solar power spectrum On the track of l=1 gravity modes
    In the present work we show robust indications of the existence of g modes in the Sun using 10 years of GOLF data. The present analysis is based on the...
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    Detection of polarization from the E4Π-A4Π system of FeH in sunspot spectra
    We report the first detection of polarization signals induced by the Zeeman Effect in lines of the E4Π-A4Π system of FeH located at 1.6 μm. Motivated by the...
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    Detection of pulsations and identification of SAX J1748.9-2021 as the X-ray transient in NGC 6440.
    On the 28th of December, MAXI/GSC detected an X-ray outburst from the globular cluster NGC6440 (Atel #2360), which has continued to the present.
  • Publicación
    Detection of second-generation asymptotic giant branch stars in metal-poor globular clusters
    Multiple stellar populations are actually known to be present in Galactic globular clusters (GCs). The first generation (FG) displays a halo-like chemical...