2007A&A...471..381Y


Query : 2007A&A...471..381Y

2007A&A...471..381Y - Astronomy and Astrophysics, volume 471381-384 (2007/8-4)

The correlations between the spin frequencies and kHz QPOs of neutron stars in LMXBs.

YIN H.X., ZHANG C.M., ZHAO Y.H., LEI Y.J., QU J.L., SONG L.M. and ZHANG F.

Abstract (from CDS):

We studied the correlations between spin frequencies and kilohertz quasi-periodic oscillations (kHz QPOs) in neutron star low-mass X-ray binaries. The updated data on kHz QPOs and spin frequencies are statistically analyzed. We find that when two simultaneous kHz QPOs are present in the power spectrum, the minimum frequency of upper kHz QPO is at least 1.3 times higher than the spin frequency, i.e. νs<ν2min/1.3. We also find that the average kHz QPO peak separation in 6 Atoll sources anti-correlates with the spin frequency in the form <Δν≥-(0.19±0.05)νs+(389.40±21.67)Hz. If we shift this correlation in the direction of the peak separation by a factor of 1.5, this correlation matches the data points of the two accretion-powered millisecond X-ray pulsars, SAX J1808.4-3658 and XTE J1807-294.

Abstract Copyright: ∼

Journal keyword(s): X-rays: binaries - accretion, accretion disks - stars: neutron

CDS comments: Paragraph 2.2 4U 1731-39 is a probable misprint for 4U 1728-34.

Simbad objects: 35

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Number of rows : 35
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* V1037 Cas LXB 00 29 03.06 +59 34 19.0           ~ 283 1
2 V* V1055 Ori LXB 06 17 07.3565603963 +09 08 13.515857360   18.80 18.5     ~ 594 1
3 V* UY Vol LXB 07 48 33.71 -67 45 07.7 16.10 17.00 16.9 16.7 17.05 ~ 660 0
4 V* BW Ant LXB 09 29 20.19 -31 23 03.2   18.50 18.63     ~ 194 0
5 V* GR Mus LXB 12 57 37.1833002949 -69 17 18.996899563   19.40 19.1     ~ 275 0
6 V* BR Cir HXB 15 20 40.8532547060 -57 10 00.206639033   21.4 21.4     B5-A0I 849 1
7 V* QX Nor LXB 16 12 43.0 -52 25 26           ~ 946 1
8 V* V818 Sco LXB 16 19 55.0692669024 -15 38 25.017666540 11.60 12.40 11.1     Oev 1730 0
9 V* V801 Ara LXB 16 40 55.5976953528 -53 45 04.948107156 17.50 18.20 17.5   17.07 ~ 921 0
10 4U 1642-45 LXB 16 45 48.1 -45 36 42           ~ 467 1
11 [KRL2007b] 214 LXB 17 00 58.46 -46 11 08.6           ~ 296 0
12 MXB 1658-298 LXB 17 02 06.54 -29 56 44.1 18.35 18.75 18.3     ~ 381 0
13 V* V1101 Sco LXB 17 05 44.4916006152 -36 25 23.049324480   20.10 18.6     ~ 473 0
14 X Ara X-1 LXB 17 06 15.2 -43 02 11           ~ 296 1
15 1RXS J170855.6-440653 LXB 17 08 54.346 -44 06 08.38           ~ 406 1
16 NAME Slow Burster LXB 17 31 58.0 -33 49 58     15.50     ~ 865 1
17 KS 1731-260 LXB 17 34 13.46 -26 05 18.6       22.8 20.9 ~ 437 0
18 V* V926 Sco LXB 17 38 58.2384053021 -44 27 00.699118812 16.90 17.70 17.5     ~ 480 0
19 SRGA J173953.4-282943 LXB 17 39 53.4 -28 29 43           ~ 106 0
20 MXB 1743-29 LXB 17 45 47 -29 17.2           ~ 54 2
21 [KRL2007b] 281 LXB 17 48 13.148 -36 07 57.02     20.9     ~ 115 0
22 [PLV2002] CX1 LXB 17 48 52.163 -20 21 32.40           ~ 213 1
23 SAX J1750.8-2900 LXB 17 50 24.42 -29 02 15.4           ~ 146 0
24 [KRL2007b] 291 LXB 17 51 13.49 -30 37 23.4           ~ 262 0
25 4U 1758-25 LXB 18 01 09.7308060816 -25 04 44.120221284     11.08     ~ 705 1
26 [KRL2007b] 304 LXB 18 06 59.8 -29 24 30           ~ 228 0
27 SAX J1808.4-3658 LXB 18 08 27.58 -36 58 43.9           ~ 1051 0
28 V* V5511 Sgr LXB 18 13 39.03 -33 46 22.3   18.61 18.33 18.05   ~ 215 0
29 V* NP Ser LXB 18 16 01.7 -14 02 09   18.8       K 683 2
30 X Sgr X-4 LXB 18 23 40.57 -30 21 40.6   19.06 18.81     ~ 1056 1
31 2MAXI J1900-248 LXB 19 00 08.65 -24 55 13.7     18.09     ~ 226 0
32 X Aql X-1 LXB 19 11 16.0571313336 +00 35 05.868232692           ~ 1186 1
33 V* V1405 Aql LXB 19 18 47.6 -05 14 18 20.90 21.40 21.0     ~ 495 0
34 V* LZ Aqr LXB 21 23 14.54 -05 47 52.9 15.90 16.78 16.8     ~ 154 0
35 V* V1341 Cyg LXB 21 44 41.1544345272 +38 19 17.066570988 15.00 15.13 14.68 15.00   A9III 1229 1

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