剑桥大学出版社期刊
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Long-Termed Variability in the Far Ultraviolet Flux of Be Stars
作者：Arne Slettebak , Theodore P. Snow
来源：[J].International Astronomical Union Colloquium, 2016, Vol.92, pp.278-281Cambridge U Press
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    The Spheroidal/Ellipsoidal, Variable Mass-Loss, Decelerated Be Star Model (Review Paper)
    作者：Arne Slettebak , Theodore P. Snow
    来源：[J].International Astronomical Union Colloquium, 2016, Vol.92, pp.384-410Cambridge U Press
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      The Short-Period Photometric Variability of Be Stars
      作者：Arne Slettebak , Theodore P. Snow
      来源：[J].International Astronomical Union Colloquium, 2016, Vol.92, pp.87-89Cambridge U Press
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        Preface
        作者：Keith S. Noll , Harold A. Weaver , Paul D. Feldman
        来源：[J].International Astronomical Union Colloquium, 2016, Vol.156, pp.xiii-xivCambridge U Press
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          The Infrared Supernova Rate
          作者：F. Mannucci , G. Cresci , R. Maiolino ...
          来源：[J].International Astronomical Union Colloquium, 2016, Vol.192, pp.355-359Cambridge U Press
          摘要：Summary Optical searches can detect supernovae (SNe) only if they suffer of a limited amount of dust extinction. This is a severe limitation as most of the core-collapse SNe could explode inside dusty regions. We describe a few ongoing projects aimed at detecting dusty SNe at nea...
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            Interstellar Absorption of Some Be Stars
            作者：Arne Slettebak , Theodore P. Snow
            来源：[J].International Astronomical Union Colloquium, 2016, Vol.92, pp.214-216Cambridge U Press
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              Optical and Near-IR Observations of SN 1998bw
              作者：Ferdinando Patat
              来源：[J].International Astronomical Union Colloquium, 2016, Vol.192, pp.381-390Cambridge U Press
              摘要：Thus, the observation of gamma-ray line emission from a young supernova seems very promising in the near future. The observation, or even a null observation at a low threshold, will give significance in the fields of nuclear astrophysics and supernova theory. The scientific impor...
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                HD 166596: A Silicon Star With Hα Emission?
                作者：Arne Slettebak , Theodore P. Snow
                来源：[J].International Astronomical Union Colloquium, 2016, Vol.92, pp.289-290Cambridge U Press
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                  Jupiter's post-impact atmospheric thermal response
                  作者：Barney J. Conrath
                  来源：[J].International Astronomical Union Colloquium, 2016, Vol.156, pp.293-306Cambridge U Press
                  摘要：Measurements of thermal emission in spectral regions, ranging from the near-infrared to mm wavelengths provide information on the atmospheric thermal structure over impact sites from μ bar levels in the upper stratosphere down to the upper troposphere. Systematic time series...
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                    Dynamics and chemistry of SL9 plumes
                    作者：Kevin Zahnle
                    来源：[J].International Astronomical Union Colloquium, 2016, Vol.156, pp.183-212Cambridge U Press
                    摘要：The SL9 impacts are known by their plumes. Several of these were imaged by HST towering 3000 km above Jupiter's limb. The heat released when they fell produced the famous infrared main events. The reentry shocks must have been significantly hotter than the observed color tem...
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