Finding fast spinning neutron stars using XMM-Newton

被引:0
|
作者
Wijnands, R. [1 ]
机构
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
来源
DECADE OF ACCRETING MILLISECOND X-RAY PULSARS | 2008年 / 1068卷
关键词
pulsars:X-ray; stars: neutron; X-ray: stars; X-ray: binaries;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The discovery of millisecond X-ray pulsations in neutron-star low-mass X-ray binaries has until now only been done with the Rossi X-ray Timing Explorer. However, XMM-Newton has also pointed at some of these systems during an outburst and shown that it can clearly detect the. pulsations as well. In fact, XMM-Newton detects the. pulsations with high enough significance to have discovered them, had they still been unknown. Thus, XMM-Newton can also be. used to search for pulsations. Moreover, for the faintest systems XMM-Newton is even more, sensitive to detect pulsations than RXTE due to the significantly less background count rate for XMM-Newton.
引用
收藏
页码:231 / 234
页数:4
相关论文
共 50 条
  • [1] The XMM-Newton view on neutron stars and black holes
    Motch, C
    INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2004, 13 (07): : 1229 - 1237
  • [2] Hot stars observed by XMM-Newton
    Nazé, Y.
    Astronomy and Astrophysics, 2009, 506 (02): : 1055 - 1064
  • [3] Constraining the neutron star equation of state using XMM-Newton
    Jonker, P. G.
    Kaastra, J.
    Mendez, M.
    In 't Zand, J. J. M.
    ASTRONOMISCHE NACHRICHTEN, 2008, 329 (02) : 198 - 201
  • [4] B stars seen at high resolution by XMM-Newton
    Cazorla, Constantin
    Naze, Yael
    ASTRONOMY & ASTROPHYSICS, 2017, 608
  • [5] A survey of young stars in the Taurus Molecular Cloud with XMM-Newton
    Güdel, M
    Briggs, K
    Telleschi, A
    Arzner, K
    Audard, M
    Grosso, N
    Bouvier, J
    Franciosini, E
    Micela, G
    Pillitteri, I
    Scelsi, L
    Stelzer, B
    Palla, F
    Padgett, D
    Rebull, L
    PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2, 2006, 604 : 39 - +
  • [6] Hot stars observed by XMM-Newton II. A survey of Oe and Be stars
    Naze, Yael
    Motch, Christian
    ASTRONOMY & ASTROPHYSICS, 2018, 619
  • [7] XMM-Newton and Geminga
    Caraveo, P
    De Luca, A
    Mereghetti, S
    Pellizzoni, A
    Bignami, G
    Tur, A
    Mignani, R
    Becker, W
    YOUNG NEUTRON STARS AND THEIR ENVIRONMENTS, 2004, (218): : 215 - 218
  • [8] A year of XMM-Newton
    Bond, P
    ASTRONOMY & GEOPHYSICS, 2001, 42 (01) : 7 - 7
  • [10] AXPs and X-ray-dim isolated neutron stars: recent XMM-Newton and Chandra results
    Haberl, F
    HIGH-ENERGY STUDIES OF SUPERNOVA REMNANTS AND NEUTRON STARS, 2004, 33 (04): : 638 - 644