2019MNRAS.489.4513S


Query : 2019MNRAS.489.4513S

2019MNRAS.489.4513S - Mon. Not. R. Astron. Soc., 489, 4513-4519 (2019/November-2)

Search for neutron star binaries in the Local Group galaxies using LISA.

SETO N.

Abstract (from CDS):

We discuss the prospects of LISA for detecting neutron star binaries (NSBs) in the Local Group galaxies such as LMC and M31. Using the recently estimated merger rate 1540 Gpc–3 yr–1 and inversely applying the conventional arguments based on the B-band galaxy luminosities, we estimate the frequency distributions of NSBs in the local galaxies. We find that, after 10 yr observation with its current design sensitivity, LISA might detect ∼5 NSBs both in LMC and M31 with signal-to-noise ratios larger than 10. Some of the NSBs might be three-dimensionally localized well within LMC. These binaries will be useful for studying various topics including the origin of r-process elements.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): gravitational waves - binaries: close

Simbad objects: 7

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Number of rows : 7
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
3 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
4 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
5 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
6 PSR J2305+4707 Psr 23 05 55.842 +47 07 45.32           ~ 227 1
7 NAME Local Group GrG ~ ~           ~ 9325 0

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