scholarly journals Cold Neutron Star Model in Brans-Dicke Theory of Gravity

1972 ◽  
Vol 48 (1) ◽  
pp. 341-343 ◽  
Author(s):  
Takuya Matsuda
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
Star Model ◽  
Theory Of Gravity

scholarly journals Neutron Star Model Atmospheres

2009 ◽  
Author(s):  
Valery Suleimanov ◽  
Thomas Rauch ◽  
Klaus Werner ◽  
Alexander Y. Potekhin ◽  
Juri Poutanen ◽  
...  
Keyword(s):  
Neutron Star ◽  
Star Model

scholarly journals Slowly rotating superfluid Newtonian neutron star model with entrainment

2002 ◽  
Vol 381 (1) ◽  
pp. 178-196 ◽  
Author(s):  
R. Prix ◽  
G. L. Comer ◽  
N. Andersson
Keyword(s):  
Neutron Star ◽  
Star Model

The maximum mass of a cold neutron star

1975 ◽  
Vol 202 ◽  
pp. 782 ◽  
Author(s):  
J. Rosen ◽  
N. Rosen
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
Maximum Mass

scholarly journals A cold neutron star in the transient low-mass X-ray binary HETE J1900.1–2455 after 10 yr of active accretion

2016 ◽  
Vol 465 (1) ◽  
pp. L10-L14 ◽  
Author(s):  
N. Degenaar ◽  
L.S. Ootes ◽  
M.T. Reynolds ◽  
R. Wijnands ◽  
D. Page
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
X Ray ◽  
Low Mass

scholarly journals Shall we Observe a Radio Binary Pulsar in SN 1987A?

1992 ◽  
Vol 128 ◽  
pp. 222-224
Author(s):  
Qiao G. J.
Keyword(s):  
Neutron Star ◽  
Surface Temperature ◽  
High Surface ◽  
Star Model ◽  
Single Star ◽  
X Ray ◽  
Binary Pulsar ◽  
Collapse Model ◽  
High Surface Temperature ◽  
Γ Ray

AbstractAn induced-collapse model [hereafter IC model; He et al. (1990)] can overcome the problems of the single star model of SN1987A. According to the IC model, there is a possibility that the SN1987A remnant will be a binary system with two neutron stars, one of them (SK-69 202) will have a strong magnetic field and a high surface temperature which favors detection as an X-ray or γ-ray pulsar. If the surface temperature of the neutron star cools down to T = 107 K, a radio binary pulsar is expected. There is also the possibility that an X-ray or γ-ray pulsar will be observed first, and only later will a radio pulsar will be detected.A newly formed neutron star is thought to have a short (millisecond) period. In this case, the core emission beam is then very large (Qiao 1992) and is thus very likely to swing in the direction of the Earth.

Binding energy and stability of a cold neutron star

1978 ◽  
Vol 225 ◽  
pp. 708 ◽  
Author(s):  
I. Goldman ◽  
N. Rosen
Keyword(s):  
Neutron Star ◽  
Binding Energy ◽  
Cold Neutron

scholarly journals Formation of Nuclear "Pasta" in Cold Neutron Star Matter

2003 ◽  
Vol 110 (4) ◽  
pp. 847-848 ◽  
Author(s):  
K. Iida ◽  
G. Watanabe ◽  
K. Sato
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
Neutron Star Matter

scholarly journals The decompression of cold neutron star matter

1977 ◽  
Vol 213 ◽  
pp. 225 ◽  
Author(s):  
J. M. Lattimer ◽  
F. Mackie ◽  
D. G. Ravenhall ◽  
D. N. Schramm
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
Neutron Star Matter
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