Tipo de publicación: Sin árbitro

  • Publicación
    Rise of the Titans: Unveiling the Nature of a Binary Hyper-Luminous Starburst at Redshift 6
    We propose HST/WFC3-IR and ACS observations in 3 bands to characterize the nature and the environment of ADFS-27, the most distant binary hyper-luminous...
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    Rmag surface brightness of HIDEEP galaxies (Minchin+, 2004)
    Optical photometry of HIDEEP galaxies was carried out using a combination of SExtractor (Bertins & Arnouts, 1996A&AS..117..393B) and the STSDAS package in IRAF...
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    Role of ISM/IGM Energy Balance in Structure Formation and Evolution of Galaxies
    Investigating the thermal and non-thermal processes in galaxies is vital to understand their evolution over cosmic time. This can best be studied by combining...
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    ROSALIA: ROman Sky Analyst for Low surface brightness Imaging & Astronomy
    Diffuse emission in the outskirts of galaxies, such as stellar tidal streams, galaxy stellar halos and intracluster light, provides important constraints on the...
  • Publicación
    Rotating Loops in the Atmosphere of Rigel (β Orionis A)
    Not Available
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    Rotating models of A and F stars (Perez Hernandez+, 1999)
    Magnitude differences between rotating and non-rotating copartners for a grid of models with solar metallicity are tabulated here. The results are expressed in...
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    Rotation and Zonal Flows in the Solar Envelope from the SOHO/MDI Observations
    We report on the latest inferences concerning solar differential rotation that have been drawn from the helioseismic data that are now available from the Solar...
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    Rotation of Hot Horizontal Branch Stars in Galactic Globular Clusters
    We present high resolution UVES+VLT spectroscopic observations of 61 stars in the extended blue horizontal branches of the Galactic globular clusters NGC 1904...
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    Rotation of the solar interior: compatibility of different helioseismic data sets
    Accurate determination of the rotation rate in the inner radiative zone (0.2 r/Rsolar 0.5) of the sun from helioseismic observations requires rotational...