-
21“... collapsing process of a high-density core, like a white dwarf or a neutron star to form a black hole. ...”
Get full text
Others -
22“... the already known pulsar period, if found, may indicate the phenomenon of neutron star oscillations, which...”
Get full text
Others -
23“... rapidly rotating neutron star. The charge depletion due to global flows of charged particles causes a...”
Get full text
Others -
24by Islam, Nazma“... the models for the mode of accretion onto the neutron star in GX 301{2: circumstellar disk model by Pravdo...”
Published 2018
Get full text
Get full text
-
25by Clark, Jason A“... accretion of hydrogen and helium from one star onto the surface of its neutron star binary companion. Mass...”
Published 2005
Get full text
Others -
26by Clark, Jason A“... accretion of hydrogen and helium from one star onto the surface of its neutron star binary companion. Mass...”
Published 2005
Get full text
-
27by Clark, Jason A“... accretion of hydrogen and helium from one star onto the surface of its neutron star binary companion. Mass...”
Published 2005
Get full text
-
28“...) composed of a neutron star and a white dwarf. The period of recurrent X-ray dips and optical modulations...”
Get full text
Others -
29“... that emission on the neutron star surface is mainly composed of a Comptonized and blackbody components...”
Get full text
Others -
30by Harstad, Emelie“... Mpc was derived for a typical neutron star-black hole coalescence progenitor assumption....”
Published 2013
Get full text
-
31by Fong, Wen-fai“... that they are the mergers of two compact objects, involving either two neutron stars (NS-NS) or a neutron star and a black...”
Published 2014
Get full text
Get full text
-
32by Das, Upasana“... in the strong gravity regime, such as, the expanding universe, the region close to a black hole and neutron star...”
Published 2018
Get full text
Get full text
-
33“... of about 10^6 ~ 10^9 Gauss for white dwarfs, 10^9 ~ 10^13 Gauss for neutron stars, and probably 10^14 ~ 10...”
Get full text
Others -
34by Hubbard, Eugene Norman“...-magnetic neutron stars, concluding that while no non-magnetic neutron stars have ever been positively...”
Published 1981
Get full text
-
35“... for the explosion of supernovae and the creation of neutron stars. The plasmon decay γ→νν is known...”
Get full text
Others -
36“...碩士 === 國立清華大學 === 天文研究所 === 105 === Magnetars are a category of neutron stars with unusually high...”
Get full text
Others -
37by Bell, Elizabeth“..., then the equilibrium ratio of protons to neutrons inside high density neutron stars can be inferred, allowing...”
Published 2005
Get full text
Others -
38by Urtekin, Kerim“... in the presence of strong magnetic fields, as is the case in the vicinities of white dwarfs and neutron stars. We...”
Published 2007
Get full text
Others -
39by Stone, Nicholas Chamberlain“... the disruption of neutron stars (NSs) by stellar mass black holes (BHs) or other NSs. Jet precession...”
Published 2013
Get full text
Get full text
-
40by Juett, Adrienne Marie, 1976-“... bibliographical references (p. 125-144). === I present high-resolution X-ray grating spectroscopy of neutron stars...”
Published 2005
Get full text
Others
