Two planets orbiting the recently formed post-common envelope binary NN Serpentis
摘要:
The eclipsing white dwarf plus main-sequence binary NN Serpentis provides one of the most convincing cases for the existence of circumbinary planets around evolved binaries. The exquisite timing precision provided by the deep eclipse of the white dwarf has revealed complex variations in the eclipse arrival times over the last few decades. These variations have been interpreted as the influence...
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关键词:
binaries: eclipsing planetary systems stars: individual: NN Ser novae cataclysmic variables planets and satellites: formation stars: evolution
DOI:
10.1051/0004-6361/201015472
被引量:
年份:
2010







































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