Kilohertz quasi-periodic intensity oscillations from 4U 1636-536

被引：58

作者：

Zhang, W

Lapidus, I

White, NE

Titarchuk, L

机构：

[1] UNIV SPACE RES ASSOC, WASHINGTON, DC USA

[2] UNIV CAMBRIDGE, INST ASTRON, CAMBRIDGE CB3 0HA, ENGLAND

[3] GEORGE MASON UNIV, COMPUTAT SCI & INFORMAT INS, FAIRFAX, VA 22030 USA

来源：

ASTROPHYSICAL JOURNAL | 1996年 / 469卷 / 01期

关键词：

binaries; general; stars; individual; (4U; 1636-536); neutron; X-rays;

D O I：

10.1086/310255

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the discovery of 870 Hz quasi-periodic intensity oscillations with the Rossi X-Ray Timing Explorer from the X-ray burster 4U 1636-536. This is the fourth Galactic low-mass X-ray binary (LMXB) that has shown this type of oscillations. We present the fractional rms amplitude as a function of energy and compare the characteristics of these oscillations with those discovered in other sources.

引用

页码：L17 / L19

页数：3

共 16 条

[1] IS GX5-1 A MILLISECOND PULSAR
ALPAR, MA
SHAHAM, J
[J]. NATURE, 1985, 316 (6025) : 239 - 241
[2] BERGER M, 1994, ASTRON ASTROPHYS, V292, P175
[3] HASINGER G, 1989, ASTRON ASTROPHYS, V225, P79
[4] Lewin W. H., 1993, SPACE SCI REV, V62, P223, DOI DOI 10.1007/BF00196124
[5] QUASI-PERIODIC OSCILLATIONS IN THE X-RAY FLUX OF THE RAPID BURSTER (MXB-1730-335)
STELLA, L
HABERL, F
LEWIN, WHG
PARMAR, AN
VANPARADIJS, J
WHITE, NE
[J]. ASTROPHYSICAL JOURNAL, 1988, 324 (01) : 379 - &
[6] STROHMAYER T, 1996, 6320 IAU
[7] Stability of r- and g-modes in neutron stars: Steady state thermonuclear excitation
Strohmayer, TE
Lee, U
[J]. ASTROPHYSICAL JOURNAL, 1996, 467 (02) : 773 - 781
[8] TITARCHUCK L, 1996, UNPUB APJL
[9] van der Klis M., 1995, X-Ray Binaries, P252
[10] van Paradijs J., 1996, 6336 IAU

← 1 2 →