剑桥大学出版社期刊
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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...
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...
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...
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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