Appearance of innermost stable circular orbits of accretion discs around rotating neutron stars

@article{42940,
   author = {Adámek, Karel and Török, Gabriel and Urbancová, Gabriela and Urbanec, Martin},
   article_location = {FR - Francouzská republika},
   article_number = {April},
   doi = {http://dx.doi.org/10.1051/0004-6361/201423541},
   keywords = {accretion accretion disks; stars: neutron; X-rays: binaries},
   language = {eng},
   issn = {0004-6361},
   journal = {Astronomy & Astrophysics},
   title = {Appearance of innermost stable circular orbits of accretion discs around rotating neutron stars},
   url = {http://www.aanda.org/articles/aa/abs/2014/04/aa23541-14/aa23541-14.html},
   volume = {564},
   year = {2014}
}

TY  - JOUR
ID  - 42940
AU  - Adámek, Karel - Török, Gabriel - Urbancová, Gabriela - Urbanec, Martin
PY  - 2014
TI  - Appearance of innermost stable circular orbits of accretion discs around rotating neutron stars
JF  - Astronomy & Astrophysics
VL  - 564
IS  - April
SP  - "L5 - 1"-"L5 - 4"
EP  - "L5 - 1"-"L5 - 4"
SN  - 00046361
KW  - accretion accretion disks
KW  - stars: neutron
KW  - X-rays: binaries
UR  - http://www.aanda.org/articles/aa/abs/2014/04/aa23541-14/aa23541-14.html
N2  - The innermost stable cicular orbit (IS(X)) of an accretion disc that orbits a neutron star (NS) is often assumed to be a unique prediction of general relativity. However, it has been argued that ISCO also appears around highly elliptic bodies described by Newtonian theory. In this sense, the behaviour of an ISCO around a rotating oblate neutron star is formed by the interplay between relativistic and Newtonian effects. Here we briefly explore the consequences of this interplay using a straightforward analytic approach as well as numerical models that involve modern NS equations of state. We examine the ratio K between the ISCO radius and the radius of the neutron star. We find that, with growing NS spin, the ratio K first decreases, but then starts toincrease. This non-monotonic behaviour of K can give rise to a neutron star spin interval in which ISCO appears for two very different ranges of NS mass. This may strongly affect the distribution of neutron stars that have an ISCO (ISCO-N
ER  - 

ADÁMEK, Karel, Gabriel TÖRÖK, Gabriela URBANCOVÁ a Martin URBANEC. Appearance of innermost stable circular orbits of accretion discs around rotating neutron stars. \textit{Astronomy \&{} Astrophysics}. FR - Francouzská republika, 2014, roč.~564, April, s.~''L5 - 1''-''L5 - 4'', 4 s. ISSN~0004-6361. Dostupné z: https://dx.doi.org/10.1051/0004-6361/201423541.