On the formation of neutron stars via accretion-induced collapse in binaries

被引:52
|
作者
Ruiter, A. J. [1 ,2 ,3 ]
Ferrario, L. [4 ]
Belczynski, K. [5 ]
Seitenzahl, I. R. [1 ,2 ]
Crocker, R. M. [2 ]
Karakas, A. I. [6 ]
机构
[1] Univ New South Wales, Sch Phys Environm & Math Sci, Australian Def Force Acad, Canberra, ACT 2600, Australia
[2] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 0200, Australia
[3] ARC Ctr Excellence All Sky Astrophys CAASTRO, Sydney, NSW, Australia
[4] Australian Natl Univ, Inst Math Sci, Canberra, ACT 0200, Australia
[5] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland
[6] Monash Univ, Sch Phys & Astron, Monash Ctr Astrophys, Clayton, Vic 3800, Australia
基金
澳大利亚研究理事会;
关键词
gravitational waves; binaries: close; stars: evolution; stars: neutron; white dwarfs; x-rays: binaries; GRAVITATIONAL-WAVE SOURCE; COMMON ENVELOPE PHASE; DOUBLE WHITE-DWARFS; IA SUPERNOVAE; MILLISECOND PULSARS; MASS-TRANSFER; DOUBLE DETONATIONS; FAINT TYPE; EVOLUTION; HELIUM;
D O I
10.1093/mnras/stz001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate evolutionary pathways leading to neutron star (NS) formation through the collapse of oxygen-neon white dwarf (ONe WD) stars in interacting binaries. We consider (1) non-dynamical mass transfer where an ONe WI) approaches the Chandrasekhar mass leading to accretion-induced collapse (AIC) and (2) dynamical time-scale merger-induced collapse (MIC) between an ONe WD and another WD. We present rates, delay times, and progenitor properties for two different treatments of common envelope evolution. We show that AIC NSs are formed via many different channels and the most dominant channel depends on the adopted common envelope physics. Most AIC and MIC NSs are born shortly after star formation, though some have delay times >10 Gyr. The shortest delay time (25-50 Myr) AIC NSs have stripped-envelope, compact, helium-burning star donors, though many prompt AIC NSs form via wind accretion from an asymptotic giant branch star. The longest delay time AIC NSs, which may be observed as young millisecond pulsars among globular clusters, have a red giant or main-sequence donor at the time of NS formation and will eventually evolve into NS + helium WD binaries. We discuss AIC and MIC binaries as potential gravitational wave sources for Laser Interferometer Space Antenna (LISA). NSs created via AIC undergo a low-mass X-ray binary phase, offering an electromagnetic counterpart for those shortest orbital period sources that LISA could identify. The formation of NSs from interacting WDs in binaries is likely to be a key mechanism for the production of LIGO/Virgo gravitational wave sources (NS-NS and BH-NS mergers) in globular clusters.
引用
收藏
页码:698 / 711
页数:14
相关论文
共 50 条
  • [1] Formation of redbacks via accretion-induced collapse
    Smedley, Sarah L.
    Tout, Christopher A.
    Ferrario, Lilia
    Wickramasinghe, Dayal T.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 446 (03) : 2540 - 2549
  • [2] The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries
    Bo Wang
    Dongdong Liu
    [J]. Research in Astronomy and Astrophysics, 2020, 20 (09) : 3 - 26
  • [3] The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries
    Wang, Bo
    Liu, Dongdong
    [J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2020, 20 (09)
  • [4] The formation of single neutron stars from double white-dwarf mergers via accretion-induced collapse
    Liu, D.
    Wang, B.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 494 (03) : 3422 - 3431
  • [5] Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei
    Perna, Rosalba
    Tagawa, Hiromichi
    Haiman, Zoltan
    Bartos, Imre
    [J]. ASTROPHYSICAL JOURNAL, 2021, 915 (01):
  • [6] Models of rapidly rotating neutron stars: remnants of accretion-induced collapse
    Liu, YT
    Lindblom, L
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 324 (04) : 1063 - 1073
  • [7] Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars?
    Chen, Hai-Liang
    Tauris, Thomas M. M.
    Chen, Xuefei
    Han, Zhanwen
    [J]. ASTROPHYSICAL JOURNAL, 2023, 951 (02):
  • [8] Multidimensional simulations of the accretion-induced collapse of white dwarfs to neutron stars
    Dessart, L.
    Burrows, A.
    Ott, C. D.
    Livne, E.
    Yoon, S. -Y.
    Langer, N.
    [J]. ASTROPHYSICAL JOURNAL, 2006, 644 (02): : 1063 - 1084
  • [9] Accretion-induced collapse to third family compact stars as trigger for eccentric orbits of millisecond pulsars in binaries
    Alvarez-Castillo, David Edwin
    Antoniadis, John
    Ayriyan, Alexander
    Blaschke, David
    Danchev, Victor
    Grigorian, Hovik
    Khosravi Largani, Noshad
    Weber, Fridolin
    [J]. ASTRONOMISCHE NACHRICHTEN, 2019, 340 (9-10) : 878 - 884
  • [10] NEUTRON-STARS AND MILLISECOND PULSARS FROM ACCRETION-INDUCED COLLAPSE IN GLOBULAR-CLUSTERS
    BAILYN, CD
    GRINDLAY, JE
    [J]. ASTROPHYSICAL JOURNAL, 1990, 353 (01): : 159 - 167