2009ApJ...694L..95E

Query : 2009ApJ...694L..95E

2009ApJ...694L..95E - Astrophys. J., 694, L95-L97 (2009/April-1)

Constraints on nonluminous matter from higher order pulsar period derivatives.

EICHLER D.

Abstract (from CDS):

Pulsar timing can detect the discreteness of the mass distribution in the Galaxy. The jerk imposed on millisecond pulsars by their nearest neighbors, and on the Sun by its nearest neighbor, may be detectable presently or within a decade. The method can detect planets in the outer solar system out to distances of several thousand AU, with the sensitivity rapidly increasing with time.

Abstract Copyright: ∼

Journal keyword(s): pulsars: general

Simbad objects: 4

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Number of rows : 4
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 J0437-47 Psr 04 37 15.7994581776 -47 15 08.544351636           DC 1032 0
2 * alf Cen ** 14 39 36.50 -60 50 02.3   0.4 -0.1     G2V+K1V 1031 0
3 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
4 PSR B1937+21.4 Psr 19 39 38.560096 +21 34 59.13552           ~ 1142 0

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