1996A&AS..120C.115R


Query : 1996A&AS..120C.115R

1996A&AS..120C.115R - Astron. Astrophys., Suppl. Ser., 120C, 115-116 (1996/December-3)

PSR B0656+14 in relation to other high-energy gamma-ray pulsars.

RAMANAMURTHY P.V., FICHTEL C.E., HARDING A.K., KNIFFEN D.A., SREEKUMAR P. and THOMPSON D.J.

Abstract (from CDS):

Possible evidence has been found for a seventh high energy gamma ray pulsar, PSR B0656+14, pulsating in gamma rays at E≥50MeV with the same 384.9ms periodicity as in radio, using the data obtained during April, 1991 to December, 1993 by the Energetic Gamma Ray Experiment Telescope (EGRET) aboard the Compton Gamma Ray Observatory (Ramanamurthy et al. 1996ApJ...458..755R). The pulsar appears to have an efficiency ∼0.001 in converting its spin-down energy loss rate into high energy gamma-rays at E≥100MeV. This efficiency is inconsistent with a general trend found for the other six pulsars seen by EGRET.

Abstract Copyright: ∼

Journal keyword(s): pulsars: individual: PSR 0656+14 - gamma-rays: observations

CDS comments: Special Issue "3rd Compton Symposium"

Simbad objects: 10

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Number of rows : 10
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 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
2 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
3 PSR J0633+1746 Psr 06 33 54.153 +17 46 12.91           ~ 1308 0
4 PSR B0656+14 Psr 06 59 48.18800 +14 14 19.2000   24.85 24.90     ~ 943 1
5 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2446 1
6 PSR B0950+08 Psr 09 53 09.31210 +07 55 36.9000           ~ 806 2
7 PSR B1055-52 Psr 10 57 59.0450 -52 26 56.330           ~ 757 0
8 PSR B1706-44 Psr 17 09 42.62000 -44 29 12.0000     13.30     ~ 670 1
9 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 801 0
10 PSR B1951+32 Psr 19 52 58.181 +32 52 40.98           ~ 615 2

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