Hunting for Dwarf Galaxies Hosting the Formation and Coalescence of Compact Binaries

被引:2
作者
Graziani, Luca [1 ,2 ,3 ]
机构
[1] Sapienza Univ Roma, Dipartimento Fis, Piazzale Aldo Moro 5, I-00185 Rome, Italy
[2] Ist Nazl Fis Nucl, Sez Roma 1, Ple Aldo Moro 2, I-00185 Rome, Italy
[3] INAF Osservatorio Astrofis Arcetri, Largo E Femi 5, I-50125 Florence, Italy
来源
PHYSICS | 2019年 / 1卷 / 03期
关键词
galaxy formation; galaxy evolution; dwarf galaxies; compact binary systems; multi-messenger astronomy; BLACK-HOLE BINARIES; STAR-FORMATION RATE; MILKY-WAY; DIFFERENT METALLICITIES; RADIATIVE-TRANSFER; MERGER RATE; MASS; EVOLUTION; POPULATION; DARK;
D O I
10.3390/physics1030030
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Here we introduce the latest version of the GAMESH model, capable to consistently account for the formation and evolution of compact binary systems along the cosmic assembly of a Milky Way (MW)-like galaxy, centered on a local group volume resolving a large population of dwarf satellites. After describing the galaxy assembly process and how the formation of binary systems is accounted for, we summarize some recent findings on the properties and evolution of low-metallicity dwarf galaxies hosting the birth/coalescence of stellar/compact binaries generating GW150914-like signals. Finally, we focus on the mass and orbital properties of the above compact binary candidates assessing their impact on the resulting coalescence times and on selecting suitable galaxy hosts.
引用
收藏
页码:412 / 429
页数:18
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