The radiative equilibrium of a spherical planetary nebula.
نویسندگان
چکیده
منابع مشابه
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Context. The evolution of stars and planets is mostly controlled by the properties of their atmosphere. This is particularly true in the case of exoplanets close to their stars, for which one has to account both for an (often intense) irradiation flux, and from an intrinsic flux responsible for the progressive loss of the inner planetary heat. Aims. The goals of the present work are to help und...
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ژورنال
عنوان ژورنال: The Astronomical Journal
سال: 1949
ISSN: 0004-6256
DOI: 10.1086/106227