Tipo de publicación: Sin árbitro

  • Publicación
    Sub-Neptune Atmospheres at High Resolution with ANDES: Can We Observe Robust Signals?
    The most probable outcome of planetary formation is a sub-Neptune, a body with a radius between 2.0 and 3.5 Earth radii. This type of exoplanet has no...
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    Sub-Stellar Binary Fraction in the Pleiades
    Not Available
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    Sub-stellar birth rate from UKIDSS (Day-Jones+, 2013)
    We select our sample from DR7 of the ULAS, selecting objects with declination
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    Subarcsecond Hα Structure of IRAS:17423-1755 and IRAS:17395-0841
    Not Available
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    Subarcsecond knots and filaments in the molecular hydrogen of the bipolar PN NGC 2346
    We present high spatial resolution (~60-90 milliarcseconds) images of the molecular hydrogen emission in the planetary nebula NGC 2346. Molecular hydrogen...
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    Subject: GRB040624, optical observations.
    Not Available
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    Submillimetre wave astronomy
    Observations in the 100-1000-micron band and the instruments used to obtain them are discussed in contributions to the Submillimeter Wave Astronomy Conference...
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    Submillimetre wave astronomy. Proceedings of a conference held at Queen Mary College, London, September 1981.
    Not Available
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    Successful Inversion of the Stellar Statistics Equation Applied to the Galactic Bulge
    Not Available