2010MNRAS.403.1978H

Query : 2010MNRAS.403.1978H

2010MNRAS.403.1978H - Mon. Not. R. Astron. Soc., 403, 1978-1982 (2010/April-3)

A resonance model with magnetic connection for 3:2 HFQPO pairs in black hole binaries.

HUANG C.-Y., GAN Z.-M., WANG J.-Z. and WANG D.-X.

Abstract (from CDS):

We apply epicyclic resonances to the magnetic connection (MC) of a black hole (BH) with a relativistic accretion disc, interpreting the high-frequency quasi-periodic oscillations (HFQPOs) with 3:2 pairs observed in three BH X-ray binaries. It turns out that the 3:2 HFQPO pairs are associated with the steep power-law states, and the severe damping can be overcome by transferring energy and angular momentum from a spinning BH to the inner disc in the MC process.

Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS

Journal keyword(s): accretion, accretion discs - black hole physics - magnetic fields - stars: individual: GRO J1655-40 - stars: individual: GRS 1915+105 - stars: individual: XTE J1550-564

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000           K3III 1254 0
2 V* V1033 Sco HXB 16 54 00.1423963019 -39 50 44.761701340       16.14   F3-6IV 1980 0
3 NAME XTE J17464-3213 LXB 17 46 15.59637 -32 14 00.8600           ~ 805 0
4 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2810 0

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