Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres.

التفاصيل البيبلوغرافية
العنوان: Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres.
المؤلفون: Gopka, Vera F., Ulyanov, Oleg M., Andrievsky, Sergey M.
المصدر: AIP Conference Proceedings; 5/21/2008, Vol. 1016 Issue 1, p460-462, 3p
مصطلحات موضوعية: NEUTRON stars, STARS, POSITRON annihilation, NUCLIDES, RADIOISOTOPES
مستخلص: We propose a new explanation of some magnetic chemically peculiar (MCP) star anomalies, which is based on an assumption that such stars be the close binary systems with a secondary component being a neutron star. Within this hypothesis one can naturally explain the main anomalous features of MCP stars: first of all, an existence of the short-lived radioactive isotopes detected in some stars (like Przybylski's star (PS) and HR465), and some others peculiarities. Also we can assume the presence of the electron-positron annihilation emission lines (0.511 MeV) in the gamma spectrum of some MCP stars. [ABSTRACT FROM AUTHOR]
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قاعدة البيانات: Complementary Index
الوصف
تدمد:0094243X
DOI:10.1063/1.2943626