Egret high-energy gamma-ray pulsar studies. I. Young spin-powered pulsars

D. J. Thompson; Z. Arzoumanian; D. L. Bertsch; K. T.S. Brazier; J. Chiang; N. D'Amico; B. L. Dingus; J. A. Esposito; J. M. Fierro; C. E. Fichtel; R. C. Hartman; S. D. Hunter; S. Johnston; G. Kanbach; V. M. Kaspi; D. A. Kniffen; Y. C. Lin; A. G. Lyne; R. N. Manchester; J. R. Mattox; H. A. Mayer-Hasselwander; P. F. Michelson; C. Von Montigny; H. I. Nel; D. J. Nice; P. L. Nolan; P. V. Ramanamurthy; S. L. Shemar; E. J. Schneid; P. Sreekumar; J. H. Taylor

doi:10.1086/174895

Egret high-energy gamma-ray pulsar studies. I. Young spin-powered pulsars

D. J. Thompson^*, Z. Arzoumanian, D. L. Bertsch, K. T.S. Brazier, J. Chiang, N. D'Amico, B. L. Dingus, J. A. Esposito, J. M. Fierro, C. E. Fichtel, R. C. Hartman, S. D. Hunter, S. Johnston, G. Kanbach, V. M. Kaspi, D. A. Kniffen, Y. C. Lin, A. G. Lyne, R. N. Manchester, J. R. MattoxH. A. Mayer-Hasselwander, P. F. Michelson, C. Von Montigny, H. I. Nel, D. J. Nice, P. L. Nolan, P. V. Ramanamurthy, S. L. Shemar, E. J. Schneid, P. Sreekumar, J. H. Taylor

^*Corresponding author for this work

Manipal Centre for Natural Sciences, Manipal

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Abstract

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 ≤ E ≤ 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.

Original language	English
Pages (from-to)	229-238
Number of pages	10
Journal	Astrophysical Journal
Volume	436
Issue number	1
DOIs	https://doi.org/10.1086/174895
Publication status	Published - 20-11-1994

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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Thompson, D. J., Arzoumanian, Z., Bertsch, D. L., Brazier, K. T. S., Chiang, J., D'Amico, N., Dingus, B. L., Esposito, J. A., Fierro, J. M., Fichtel, C. E., Hartman, R. C., Hunter, S. D., Johnston, S., Kanbach, G., Kaspi, V. M., Kniffen, D. A., Lin, Y. C., Lyne, A. G., Manchester, R. N., ... Taylor, J. H. (1994). Egret high-energy gamma-ray pulsar studies. I. Young spin-powered pulsars. Astrophysical Journal, 436(1), 229-238. https://doi.org/10.1086/174895

@article{3439949f376a4edea2c563b6003b1872,

title = "Egret high-energy gamma-ray pulsar studies. I. Young spin-powered pulsars",

abstract = "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 ≤ E ≤ 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.",

author = "Thompson, \{D. J.\} and Z. Arzoumanian and Bertsch, \{D. L.\} and Brazier, \{K. T.S.\} and J. Chiang and N. D'Amico and Dingus, \{B. L.\} and Esposito, \{J. A.\} and Fierro, \{J. M.\} and Fichtel, \{C. E.\} and Hartman, \{R. C.\} and Hunter, \{S. D.\} and S. Johnston and G. Kanbach and Kaspi, \{V. M.\} and Kniffen, \{D. A.\} and Lin, \{Y. C.\} and Lyne, \{A. G.\} and Manchester, \{R. N.\} and Mattox, \{J. R.\} and Mayer-Hasselwander, \{H. A.\} and Michelson, \{P. F.\} and \{Von Montigny\}, C. and Nel, \{H. I.\} and Nice, \{D. J.\} and Nolan, \{P. L.\} and Ramanamurthy, \{P. V.\} and Shemar, \{S. L.\} and Schneid, \{E. J.\} and P. Sreekumar and Taylor, \{J. H.\}",

year = "1994",

month = nov,

day = "20",

doi = "10.1086/174895",

language = "English",

volume = "436",

pages = "229--238",

journal = "Astrophysical Journal",

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Thompson, DJ, Arzoumanian, Z, Bertsch, DL, Brazier, KTS, Chiang, J, D'Amico, 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, Mayer-Hasselwander, HA, Michelson, PF, Von Montigny, C, Nel, HI, Nice, DJ, Nolan, PL, Ramanamurthy, PV, Shemar, SL, Schneid, EJ, Sreekumar, P & Taylor, JH 1994, 'Egret high-energy gamma-ray pulsar studies. I. Young spin-powered pulsars', Astrophysical Journal, vol. 436, no. 1, pp. 229-238. https://doi.org/10.1086/174895

TY - JOUR

T1 - Egret high-energy gamma-ray pulsar studies. I. Young spin-powered pulsars

AU - Thompson, D. J.

AU - Arzoumanian, Z.

AU - Bertsch, D. L.

AU - Brazier, K. T.S.

AU - Chiang, J.

AU - D'Amico, N.

AU - Dingus, B. L.

AU - Esposito, J. A.

AU - Fierro, J. M.

AU - Fichtel, C. E.

AU - Hartman, R. C.

AU - Hunter, S. D.

AU - Johnston, S.

AU - Kanbach, G.

AU - Kaspi, V. M.

AU - Kniffen, D. A.

AU - Lin, Y. C.

AU - Lyne, A. G.

AU - Manchester, R. N.

AU - Mattox, J. R.

AU - Mayer-Hasselwander, H. A.

AU - Michelson, P. F.

AU - Von Montigny, C.

AU - Nel, H. I.

AU - Nice, D. J.

AU - Nolan, P. L.

AU - Ramanamurthy, P. V.

AU - Shemar, S. L.

AU - Schneid, E. J.

AU - Sreekumar, P.

AU - Taylor, J. H.

PY - 1994/11/20

Y1 - 1994/11/20

N2 - 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 ≤ E ≤ 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.

AB - 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 ≤ E ≤ 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.

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DO - 10.1086/174895

M3 - Article

AN - SCOPUS:12044252913

SN - 0004-637X

VL - 436

SP - 229

EP - 238

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

ER -

Egret high-energy gamma-ray pulsar studies. I. Young spin-powered pulsars

Abstract

All Science Journal Classification (ASJC) codes

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