EGRET HIGH-ENERGY GAMMA-RAY PULSAR STUDIES .1. YOUNG SPIN-POWERED PULSARS

被引：107

作者：

THOMPSON, DJ

ARZOUMANIAN, Z

BERTSCH, DL

BRAZIER, KTS

CHIANG, J

DAMICO, N

DINGUS, BL

ESPOSITO, JA

FIERRO, JM

FICHTEL, CE

HARTMAN, RC

HUNTER, SD

JOHNSTON, S

KANBACH, G

KASPI, VM

KNIFFEN, DA

LIN, YC

LYNE, AG

MANCHESTER, RN

MATTOX, JR

MAYERHASSELWANDER, HA

MICHELSON, PF

VONMONTIGNY, C

NEL, HI

NICE, DJ

NOLAN, PL

RAMANAMURTHY, PV

SHEMAR, SL

SCHNEID, EJ

SREEKUMAR, P

TAYLOR, JH

机构：

[1] PRINCETON UNIV, DEPT PHYS, PRINCETON, NJ 08544 USA

[2] MAX PLANCK INST EXTRATERR PHYS, D-85748 GARCHING, GERMANY

[3] STANFORD UNIV, WW HANSEN EXPTL PHYS LAB, STANFORD, CA 94305 USA

[4] STANFORD UNIV, DEPT PHYS, STANFORD, CA 94305 USA

[5] UNIV PALERMO, IST FIS, I-40126 PALERMO, ITALY

[6] CNR, IST RADIOASTRON, I-40126 BOLOGNA, ITALY

[7] CSIRO, AUSTRALIA TELESCOPE NATL FACIL, EPPING, NSW 2121, AUSTRALIA

[8] UNIV MANCHESTER, DEPT PHYS, MACCLESFIELD SK11 9DL, CHESHIRE, ENGLAND

[9] POTCHEFSTROOM UNIV CHRISTIAN HIGHER EDUC, DEPT PHYS, POTCHEFSTROOM 2520, SOUTH AFRICA

[10] GRUMMAN AEROSP CORP, BETHPAGE, NY 11714 USA

来源：

ASTROPHYSICAL JOURNAL | 1994年 / 436卷 / 01期

关键词：

GAMMA RAYS; PULSARS; GENERAL;

D O I：

10.1086/174895

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

As part of its ongoing survey of the high-energy gamma-ray sky, the Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory has searched for emission from spin-powered pulsars, five of which have now been detected in the energy range 30 MeV less than or equal to E less than or equal to 20 GeV. A systematic study of the all-sky survey has found no additional pulsed gamma-ray sources. The pulsar detections, coupled with the upper limits on pulsed gamma radiation from other radio pulsars, indicate that the simplest models of gamma-ray pulsars are incomplete.

引用

页码：229 / 238

页数：10

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