DETERMINISTIC CHAOS IN ACCRETING NEUTRON-STAR SYSTEMS

被引：0
|
作者：
MORFILL, GE
ATMANSPACHER, H
DEMMEL, V
SCHEINGRABER, H
VOGES, W
机构：
来源：
TIMING NEUTRON STARS | 1989年 / 262卷
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：
引用
收藏
页码：71 / 93
页数：23
相关论文
共 50 条
  • [31] WORKSHOP ON NEUTRON-STAR PHYSICS
    VARSHALOVICH, DA
    KAMINKER, AD
    YAKOVLEV, DG
    SOVIET ASTRONOMY LETTERS, 1992, 18 (06): : 455 - 458
  • [32] PHYSICS OF NEUTRON-STAR ENVELOPES
    DENIEM, D
    ASTRONOMISCHE NACHRICHTEN, 1986, 307 (05) : 347 - 348
  • [33] ENERGY OF NEUTRON-STAR MATTER
    MOSZKOWSKI, SA
    PHYSICAL REVIEW D, 1974, 9 (06) : 1613 - 1625
  • [34] HIGH-ENERGY X-RAY-PRODUCTION IN A BOUNDARY-LAYER OF AN ACCRETING NEUTRON-STAR
    HANAWA, T
    ASTROPHYSICAL JOURNAL, 1991, 373 (01): : 222 - 227
  • [35] Neutron-star matter within the energy-density functional theory and neutron-star structure
    Fantina, A. F.
    Chamel, N.
    Pearson, J. M.
    Goriely, S.
    EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (V). FROM NUCLEI TO STARS, 2015, 1645 : 92 - 100
  • [36] FORMATION OF DOUBLE NEUTRON-STAR SYSTEMS AND ASYMMETRIC SUPERNOVA EXPLOSIONS
    YAMAOKA, H
    SHIGEYAMA, T
    NOMOTO, K
    ASTRONOMY & ASTROPHYSICS, 1993, 267 (02) : 433 - 438
  • [37] PROTON AND NEUTRON SUPERFLUIDITY IN NEUTRON-STAR MATTER
    BALDO, M
    CUGNON, J
    LEJEUNE, A
    LOMBARDO, U
    NUCLEAR PHYSICS A, 1992, 536 (02) : 349 - 365
  • [38] Neutron-Star Radius from a Population of Binary Neutron Star Mergers
    Bose, Sukanta
    Chakravarti, Kabir
    Rezzolla, Luciano
    Sathyaprakash, B. S.
    Takami, Kentaro
    PHYSICAL REVIEW LETTERS, 2018, 120 (03)
  • [39] HIGH-PRECISION ROTATING NEUTRON-STAR MODELS .1. ANALYSIS OF NEUTRON-STAR PROPERTIES
    SALGADO, M
    BONAZZOLA, S
    GOURGOULHON, E
    HAENSEL, P
    ASTRONOMY & ASTROPHYSICS, 1994, 291 (01) : 155 - 170
  • [40] POSSIBLE SIGNATURES OF THE CONVERSION OF A NEUTRON-STAR TO A STRANGE STAR
    BENVENUTO, OG
    KRIVORUCHENKO, MI
    MARTEMYANOV, BV
    INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 1994, 3 (03): : 653 - 664
12345