Tipo de publicación: Sin árbitro

  • Publicación
    Be-9 abundances in dwarfs of intermediate metal deficiency - Implications for galactic evolution
    This paper presents observations of the 3130 A Be II resonance doublet in stars of intermediate metal deficiency, with Fe/H values between -0.6 and -1.1...
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    Be-9 abundances in halo dwarfs - Implications for early nucleosynthesis of light elements
    Not Available
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    Beam asymmetry Σ in η' photoproduction off the proton at the GRAAL experiment
    The only recent η' photoproduction data off proton available in literature are the differential and total cross sections published by the CLAS and CB-ELSA-TAPS...
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    Beam focusing of a laser guide star
    It is foreseen that Extremly large telescope (ELT) will include Adaptive Optics Systems to provide diffraction-limited images in the near infrared. The...
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    Behaviour of the H-alpha Line of V404 CYG
    We present spectroscopy of the Hα emision line in the X-ray transient V4 04 Cyg. Along with the spectroscopy, simultaneus photometry was used in order t o...
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    Behaviour of the H-α line of the black hole X-ray binary V404 CYG
    Not Available
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    Benchmark brown dwarf companions as exoplanets analogues
    Directly imaged substellar companions around stars are key objects for better understanding the formation and evolution of brown dwarfs and massive planets, as...
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    Benchmark Brown Dwarfs: What Does the Current Population Look Like?
    Since the discovery of the first brown dwarfs (Tiede 1; Rebolo et al. 1995, Gliese 229B; Nakajima et al. 1995) the complement of identified brown dwarfs has...
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    Benchmark ultra-cool dwarfs in widely separated binary systems
    Ultra-cool dwarfs as wide companions to subgiants, giants, white dwarfs and main sequence stars can be very good benchmark objects, for which we can infer...