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2“...碩士 === 國立清華大學 === 物理學系 === 91 === We develop an atmosphere model for neutron stars...”
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3“... of an early type star and a neutron star as an accretor. The orbital period of the binary is 1.4 days...”
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4“.... By the same consideration, we can compute the mass limit of the neutron star, which is 5.69...”
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5“... folded with an ephemeris consist of the neutron star spin frequency evolution plus the effect from...”
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6“... with a neutron star accreting matter from the Roche lobe-filling main-sequence star. The source...”
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7“... of possible hot spot movements on the surface of neutron star, no simple model can well-describe the pulse...”
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8“... exhibiting X-ray burst and periodic X-ray dips. Both systems consist of a neutron star as accretor and a...”
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9“... the center of the globular cluster NGC 6624, composed of a neutron star and a ~20% degeneracy white dwarf...”
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10“... ck waves, and the high-velocity outflows can be found in galactic jets,binary neutron...”
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