Zobrazeno 1 - 10
of 96
pro vyhledávání: '"Sevinc, O."'
Autor:
OZDEMIR, M., SEVINC, O. F.
Publikováno v:
European Review for Medical & Pharmacological Sciences; Apr2024, Vol. 28 Issue 8, p3263-3267, 5p
The available data on isolated X-ray pulsars, their wind nebulae, and the supernova remnants which are connected to some of these sources are analyzed. It is shown that electric fields of neutron stars tear off charged particles from the surface of n
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702571
The available data of single X-ray pulsars, their wind nebulae, and the SNRs which are connected to some of these sources are analysed. It is shown that electric field intensity of neutron stars tears off charged particles from the surface of neutron
Externí odkaz:
http://arxiv.org/abs/astro-ph/0401114
Publikováno v:
Astrophys.Space Sci.298:553-558,2005
Influences of the mass, moment of inertia, rotation, absence of stability in the atmosphere and some other parameters of neutron stars on the evolution of pulsars are examined. It is shown that the locations and evolutions of soft gamma repeaters, an
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309241
Publikováno v:
Int.J.Mod.Phys.D14:643-656,2005
We estimate the spatial densities of different types of neutron star near the Sun. It is shown that the distances of dim isolated thermal neutron stars must be on average about 300-400 pc. The combined birth rate of these sources together with radio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309133
We examined correlations between young radio pulsars (PSRs), Supernova remnants (SNRs) which have different surface brightness values and young star formation regions (SFRs). Angular correlation of PSRs with SFRs is reliable up to 4 kpc and considera
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306117
In different directions of the Galaxy the Galactic background radio radiation and radiation of complex star formation regions which include large number of OB associations have different influences on radio pulsar (PSR) and supernova remnant (SNR) se
Externí odkaz:
http://arxiv.org/abs/astro-ph/0305490
In this work, we have constructed a relation between the surface brightness ($\Sigma$) and diameter (D) of Galactic C- and S-type supernova remnants (SNRs). In order to calibrate the $\Sigma$-D dependence, we have carefully examined some intrinsic (e
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304499
Akademický článek
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Autor:
Sevinc, O.1 osevinc@istanbul.edu.tr, Gudekli, E.1
Publikováno v:
Advances in High Energy Physics. 2011, p1-10. 10p.