Gamma radiation from PSR B1055-52

被引：123

作者：

Thompson, DJ

Bailes, M

Bertsch, DL

Cordes, J

D'Amico, N

Esposito, JA

Finley, J

Hartman, RC

Hermsen, W

Kanbach, G

Kaspi, VM

Kniffen, DA

Kuiper, L

Lin, YC

Lyne, A

Manchester, R

Matz, SM

Mayer-Hasselwander, HA

Michelson, PF

Nolan, PL

Ögelman, H

Pohl, M

Ramanamurthy, PV

Sreekumar, P

Reimer, O

Taylor, JH

Ulmer, M

机构：

[1] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA

[2] Swinburne Univ Technol, Hawthorn, Vic 3122, Australia

[3] Cornell Univ, Dept Phys, Ithaca, NY 14853 USA

[4] Osservatorio Astron Bologna, I-40126 Bologna, Italy

[5] Purdue Univ, Dept Phys, Lafayette, IN USA

[6] SRON, NL-3584 CA Utrecht, Netherlands

[7] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[8] MIT, Dept Phys, Cambridge, MA 02139 USA

[9] Hampden Sydney Coll, Dept Phys, Hampden Sydney, VA 23943 USA

[10] Stanford Univ, WW Hansen Labs Phys, Stanford, CA 94305 USA

[11] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[12] Univ Manchester, Nuffield Radio Astron Labs, Jodrell Bank, Macclesfield SK11 9DL, Cheshire, England

[13] CSIRO, ATNF, Epping, NSW, Australia

[14] Northwestern Univ, Dept Phys, Evanston, IL 60208 USA

[15] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[16] Danish Space Res Inst, Copenhagen 2100 O, Denmark

[17] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

来源：

ASTROPHYSICAL JOURNAL | 1999年 / 516卷 / 01期

关键词：

gamma rays : observations; pulsars : individual (PSR B1055-52);

D O I：

10.1086/307083

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The telescopes on the Compton Gamma Ray Observatory (CGRO) have observed PSR B1055-52 a number of times between 1991 and 1998. From these data a more detailed picture of the gamma radiation from this source has been developed, showing several characteristics that distinguish this pulsar: the light curve is complex; there is no detectable unpulsed emission; the energy spectrum is hat, with no evidence of a sharp high-energy cutoff up to greater than 4 GeV. Comparisons of the gamma-ray data with observations at longer wavelengths show that no two of the known gamma-ray pulsars have quite the same characteristics; this diversity males interpretation in terms of theoretical models difficult.

引用

页码：297 / 306

页数：10

共 108 条

[31] EINSTEIN OBSERVATIONS OF THE CRAB-NEBULA PULSAR [J].