2001A&A...375..890N

Query : 2001A&A...375..890N

2001A&A...375..890N - Astronomy and Astrophysics, volume 375890-898 (2001/9-1)

The gravitational wave signal from the Galactic disk population of binaries containing two compact objects.

NELEMANS G., YUNGELSON L.R. and PORTEGIES ZWART S.F.

Abstract (from CDS):

We review the properties of Galactic binaries containing two compact objects, as derived by means of population synthesis. Using this information we calculate the gravitational wave signal of these binaries. At frequencies below f≲2mHz the double white dwarf population forms an unresolved background for the low-frequency gravitational wave detector LISA. Above this limit some few thousand double white dwarfs and few tens of binaries containing neutron stars will be resolved. Of the resolved double white dwarfs ∼500 have a total mass above the Chandrasekhar limit. About ∼95 of these have a measurable frequency change allowing a determination of their chirp mass. We discuss the properties of the resolved systems.

Abstract Copyright: ∼

Journal keyword(s): gravitational waves - stars: statistics - binaries: close - galaxy: stellar content

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 PSR J1915+1606 Psr 19 15 27.99999 +16 06 27.4034     22.5     ~ 1032 1

Query : 2001A&A...375..890N

Basic data :
PSR J1915+1606 -- Pulsar
Other object types: otypes_help 		SB* (SBC7,SBC9), Psr (PSR), * (WEB)
ICRS coord. (ep=J2000) : 		19 15 27.99999 +16 06 27.4034 [ ] D 2003ASPC..302...93W
FK4 coord. (ep=B1950 eq=1950) : 		19 13 12.45366 +16 01 07.9874 [ ]
Gal coord. (ep=J2000) : 		049.96765583 +02.12189140 [ ]
Fluxes (1) :
V 22.5 [~] E ~
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Identifiers (7) :
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PSR B1913+16.0 PSR B1913+16 SBC7 741 WEB 16499
NAME Hulse-Taylor PSR PSR J1915+1606 SBC9 1137

References (1032 between 1850 and 2026) (Total 1032)
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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