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تسجيل مستخدم جديدLife Cycles of Magnetic Fields in Stellar Evolution
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تأليف
D. Uzdensky
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This is a white paper submitted to the Stars and Stellar Evolution (SSE) Science Frontier Panel (SFP) of the NRCs Astronomy and Astrophysics 2010 Decadal Survey. The white paper is endorsed by the American Physical Societys (APS) Topical Group on Plasma Astrophysics (GPAP).
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Neutron stars are natural physical laboratories allowing us to study a plethora of phenomena in extreme conditions. In particular, these compact objects can have very strong magnetic fields with non-trivial origin and evolution. In many respects its
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