Extended orbital resonance model applied to QPOs observed in
three near-extreme Kerr black hole candidate systems

D 2007

Extended orbital resonance model applied to QPOs observed in three near-extreme Kerr black hole candidate systems

STUCHLÍK, Zdeněk a Petr SLANÝ

Základní údaje

Originální název

Extended orbital resonance model applied to QPOs observed in three near-extreme Kerr black hole candidate systems

Autoři

STUCHLÍK, Zdeněk a Petr SLANÝ

Vydání

Opava, Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars, od s. 257-265, 9 s. 2007

Nakladatel

Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Stát vydavatele

Česká republika

Utajení

není předmětem státního či obchodního tajemství

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

ISBN

978-80-7248-419-5

Klíčová slova anglicky

black hole physics, relativity, accretion discs, X-rays: individual:GRS 1915+105, XTE J1650-500, NGC 5408 X-1

Štítky

RAGtime, sbornik, UF

Příznaky

Mezinárodní význam

Návaznosti

MSM4781305903, záměr.

Změněno: 21. 12. 2020 11:09, Mgr. Pavlína Jalůvková

Anotace

V originále

The "Extended Orbital Resonance Model," i.e., the idea of oscillations induced by the hump of the orbital velocity profile (related to the locally non-rotating frames - LNRF), which are proposed to excite the oscillations of Keplerian discs around near-extreme Kerr black holes with epicyclic frequencies, is used to estimate the mass and spin of three near-extreme Kerr black hole candidates GRS 1915+105, XTE J1650-500, and NGC 5408 X-1. The hump-induced oscillations are characterized by the so-called "humpy frequency," and a non-linear resonant coupling between these and epicyclic oscillations is expected. It it shown that the quasiperiodic variability (QPOs) observed in these sources can be matched with the proposals of the model, giving for the mass and spin of their black holes values consistent with the other observationally-established estimates.

Citovat

STUCHLÍK, Zdeněk a Petr SLANÝ. Extended orbital resonance model applied to QPOs observed in three near-extreme Kerr black hole candidate systems. In Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars. Opava: Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky, 2007, s. 257-265. ISBN 978-80-7248-419-5.

@inproceedings{44204,
   author = {Stuchlík, Zdeněk and Slaný, Petr},
   address = {Opava},
   booktitle = {Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars},
   keywords = {black hole physics, relativity, accretion discs, X-rays: individual:GRS 1915+105, XTE J1650-500, NGC 5408 X-1},
   language = {eng},
   location = {Opava},
   isbn = {978-80-7248-419-5},
   pages = {257-265},
   publisher = {Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky},
   title = {Extended orbital resonance model applied to QPOs observed in three near-extreme Kerr black hole candidate systems},
   year = {2007}
}

TY  - CONF
ID  - 44204
AU  - Stuchlík, Zdeněk - Slaný, Petr
PY  - 2007
TI  - Extended orbital resonance model applied to QPOs observed in three near-extreme Kerr black hole candidate systems
PB  - Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
CY  - Opava
SN  - 9788072484195
KW  - black hole physics, relativity, accretion discs, X-rays: individual:GRS 1915+105, XTE J1650-500, NGC 5408 X-1
N2  - The "Extended Orbital Resonance Model," i.e., the idea of oscillations induced by the hump of the orbital velocity profile (related to the locally non-rotating frames - LNRF), which are proposed to excite the oscillations of Keplerian discs around near-extreme Kerr black holes with epicyclic frequencies, is used to estimate the mass and spin of three near-extreme Kerr black hole candidates GRS 1915+105, XTE J1650-500, and NGC 5408 X-1. The hump-induced oscillations are characterized by the so-called "humpy frequency," and a non-linear resonant coupling between these and epicyclic oscillations is expected. It it shown that the quasiperiodic variability (QPOs) observed in these sources can be matched with the proposals of the model, giving for the mass and spin of their black holes values consistent with the other observationally-established estimates.
ER  -

STUCHLÍK, Zdeněk a Petr SLANÝ. Extended orbital resonance model applied to QPOs observed in three near-extreme Kerr black hole candidate systems. In \textit{Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars}. Opava: Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky, 2007, s.~257-265. ISBN~978-80-7248-419-5.

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