2017MNRAS.469..930C

Query : 2017MNRAS.469..930C

2017MNRAS.469..930C - Mon. Not. R. Astron. Soc., 469, 930-937 (2017/July-3)

LISA detection of binary black holes in the Milky Way galaxy.

CHRISTIAN P. and LOEB A.

Abstract (from CDS):

Using the black hole merger rate inferred from LIGO, we calculate the abundance of tightly bound binary black holes in the Milky Way galaxy. Binaries with a small semimajor axis (<=10 R☉) originate at larger separations through conventional formation mechanisms and evolve as a result of gravitational wave emission. We find that LISA could detect them in the Milky Way. We also identify possible X-ray signatures of such binaries.

Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): gravitational waves - binaries: general - X-rays: binaries - X-rays: binaries

Simbad objects: 1

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Number of rows : 1
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 GrW 150914 GWE ~ ~           ~ 674 1

Query : 2017MNRAS.469..930C

Basic data :
GrW 150914 -- Gravitational Wave Event
Other object types: otypes_help 		GWE (GrW)
ICRS coord. (ep=J2000) : 		No Coord.
Radial velocity / Redshift / cz : 		V(km/s) 25772 [~] / z(~) 0.09 [~] / cz 26981 [~]
   E 2016ApJ...823L..25K
notes:

Identifiers (3) :
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GrW 150914 095045 GrW 150914 NAME GW150914

References (674 between 1850 and 2026) (Total 674)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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