On the bottom magnetic fields of millisecond pulsars

被引：0
|
作者：
Mang, CM [1 ]
机构：
[1] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
来源：
YOUNG NEUTRON STARS AND THEIR ENVIRONMENTS | 2004年 / 218期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The magnetic field strengths of most millisecond pulsars (MSPs) are about 10(8-9) gauss. The accretion-induced magnetic field evolution scenario here concludes that field decay is related to the accreted mass, that the minimum or bottom field stops at about 10(8) gauss for Eddington-limited accretion, and scales with the accretion rate as M-1/2. The possibility of low field (similar to 10(7) gauss) MSPs has been proposed for future radio observations.
引用
收藏
页码：47 / 48
页数：2
相关论文
共 50 条
  • [41] Deep optical observations of the fields of two nearby millisecond pulsars with the VLT
    Sutaria, F.K.
    Ray, A.
    Reisenegger, A.
    Hertling, G.
    Quintana, H.
    Minniti, D.
    Astronomy and Astrophysics, 2003, 406 (01): : 245 - 252
  • [42] Binary and Millisecond Pulsars
    Lorimer, Duncan R.
    LIVING REVIEWS IN RELATIVITY, 2008, 11 (1)
  • [43] THE BINARY AND MILLISECOND PULSARS
    GRAHAMSMITH, F
    CONTEMPORARY PHYSICS, 1992, 33 (03) : 165 - 173
  • [44] Timing of millisecond pulsars
    Backer, DC
    COMPACT STARS IN BINARIES, 1996, (165): : 197 - 211
  • [45] On the origin of millisecond pulsars
    Urpin, V
    Geppert, U
    Konenkov, D
    ASTRONOMY & ASTROPHYSICS, 1998, 331 (01) : 244 - 250
  • [46] ASTROMETRY OF MILLISECOND PULSARS
    TAYLOR, JH
    HIGHLIGHTS OF ASTRONOMY, VOL 8, 1989, : 471 - 472
  • [47] ORIGIN OF MILLISECOND PULSARS
    MICHEL, FC
    NATURE, 1987, 329 (6137) : 310 - 312
  • [48] Binary and Millisecond Pulsars
    Duncan R. Lorimer
    Living Reviews in Relativity, 2005, 8
  • [49] HIDDEN MILLISECOND PULSARS
    TAVANI, M
    ASTROPHYSICAL JOURNAL, 1991, 379 (02): : L69 - L73
  • [50] BINARY AND MILLISECOND PULSARS
    PHINNEY, ES
    KULKARNI, SR
    ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1994, 32 : 591 - 639
12345