Tipo de publicación: Sin árbitro

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    Multiple Components to XY UMa Light
    Not Available
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    Multiple Quasars: Theory VS. Observations
    Not Available
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    Multiple Sequences of M-dwarfs in NGC 2808 and ω Centauri.
    The infrared channel of the Wide-Field Camera 3 on the Hubble Space Telescope revealed multiple main sequences of very low-mass stars in the globular clusters...
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    Multiple Star Systems in the Orion Nebula
    GRAVITY observations reveal that most massive stars in the Orion Trapezium cluster live in multiple systems. Our deep, milliarcsecond-resolution interferometry...
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    Multiple stellar generations in the Large Magellanic Cloud Star Cluster NGC 1846
    The recent discovery of multiple stellar populations in massive Galactic globular clusters poses a serious challenge for models of star cluster formation and...
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    Multiple stellar populations in Galactic globular clusters: observational evidence
    An increasing number of both photometric and spectroscopic observations over the last years have shown the existence of distinct sub-populations in many...
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    Multiple stellar populations in the Globular Clusters NGC1851 and NGC6656 (M22).
    In the last years, photometric and spectroscopic evidence has demonstrated that many, maybe all the Globular Clusters (GC) host multiple stellar populations...
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    Multiplicity Among Young Brown Dwarfs and Very Low Mass Stars
    Characterizing multiplicity in the very low mass (VLM) domain is a topic of much current interest and fundamental importance. Here we report on a near-infrared...
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    Multiplicity at the Very Low Mass End of the H-R Diagram
    We review the properties of multiplicity of very low mass stars and brown dwarfs in different environments and at different ages. We will compare the main...