Gamma radiation from PSR B1055-52

D. J. Thompson; M. Bailes; D. L. Bertsch; J. Cordes; N. D'Amico; J. A. Esposito; J. Finley; R. C. Hartman; W. Hermsen; G. Kanbach; V. M. Kaspi; D. A. Kniffen; L. Kuiper; Y. C. Lin; A. Lyne; R. Manchester; S. M. Matz; H. A. Mayer-Hasselwander; P. F. Michelson; P. L. Nolan; H. Ögelman; M. Pohl; P. V. Ramanamurthy; P. Sreekumar; O. Reimer; J. H. Taylor; M. Ulmer

doi:10.1086/307083

Gamma radiation from PSR B1055-52

D. J. Thompson^*
, M. Bailes
, D. L. Bertsch
, J. Cordes
, N. D'Amico
, J. A. Esposito
, J. Finley
, R. C. Hartman
, W. Hermsen
, G. Kanbach
, V. M. Kaspi
, D. A. Kniffen
, L. Kuiper
, Y. C. Lin
, A. Lyne
, R. Manchester
, S. M. Matz
, H. A. Mayer-Hasselwander
, P. F. Michelson
, P. L. Nolan

H. Ögelman, M. Pohl, P. V. Ramanamurthy, P. Sreekumar, O. Reimer, J. H. Taylor, M. Ulmer

^*Corresponding author for this work

Manipal Centre for Natural Sciences, Manipal

Research output: Contribution to journal › Article › peer-review

108 Citations (Scopus)

Abstract

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 flat, 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 makes interpretation in terms of theoretical models difficult.

Original language	English
Pages (from-to)	297-306
Number of pages	10
Journal	Astrophysical Journal
Volume	516
Issue number	1 PART 1
DOIs	https://doi.org/10.1086/307083
Publication status	Published - 01-05-1999

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/307083

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Thompson, D. J., Bailes, M., Bertsch, D. L., Cordes, J., D'Amico, N., Esposito, J. A., Finley, J., Hartman, R. C., Hermsen, W., Kanbach, G., Kaspi, V. M., Kniffen, D. A., Kuiper, L., Lin, Y. C., Lyne, A., Manchester, R., Matz, S. M., Mayer-Hasselwander, H. A., Michelson, P. F., ... Ulmer, M. (1999). Gamma radiation from PSR B1055-52. Astrophysical Journal, 516(1 PART 1), 297-306. https://doi.org/10.1086/307083

@article{129273ac3e274c339713bbfd4c88465a,

title = "Gamma radiation from PSR B1055-52",

abstract = "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 flat, 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 makes interpretation in terms of theoretical models difficult.",

author = "Thompson, \{D. J.\} and M. Bailes and Bertsch, \{D. L.\} and J. Cordes and N. D'Amico and Esposito, \{J. A.\} and J. Finley and Hartman, \{R. C.\} and W. Hermsen and G. Kanbach and Kaspi, \{V. M.\} and Kniffen, \{D. A.\} and L. Kuiper and Lin, \{Y. C.\} and A. Lyne and R. Manchester and Matz, \{S. M.\} and Mayer-Hasselwander, \{H. A.\} and Michelson, \{P. F.\} and Nolan, \{P. L.\} and H. {\"O}gelman and M. Pohl and Ramanamurthy, \{P. V.\} and P. Sreekumar and O. Reimer and Taylor, \{J. H.\} and M. Ulmer",

year = "1999",

month = may,

day = "1",

doi = "10.1086/307083",

language = "English",

volume = "516",

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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 1999, 'Gamma radiation from PSR B1055-52', Astrophysical Journal, vol. 516, no. 1 PART 1, pp. 297-306. https://doi.org/10.1086/307083

TY - JOUR

T1 - Gamma radiation from PSR B1055-52

AU - Thompson, D. J.

AU - Bailes, M.

AU - Bertsch, D. L.

AU - Cordes, J.

AU - D'Amico, N.

AU - Esposito, J. A.

AU - Finley, J.

AU - Hartman, R. C.

AU - Hermsen, W.

AU - Kanbach, G.

AU - Kaspi, V. M.

AU - Kniffen, D. A.

AU - Kuiper, L.

AU - Lin, Y. C.

AU - Lyne, A.

AU - Manchester, R.

AU - Matz, S. M.

AU - Mayer-Hasselwander, H. A.

AU - Michelson, P. F.

AU - Nolan, P. L.

AU - Ögelman, H.

AU - Pohl, M.

AU - Ramanamurthy, P. V.

AU - Sreekumar, P.

AU - Reimer, O.

AU - Taylor, J. H.

AU - Ulmer, M.

PY - 1999/5/1

Y1 - 1999/5/1

N2 - 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 flat, 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 makes interpretation in terms of theoretical models difficult.

AB - 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 flat, 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 makes interpretation in terms of theoretical models difficult.

UR - https://www.scopus.com/pages/publications/0033126002

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SN - 0004-637X

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SP - 297

EP - 306

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 PART 1

ER -

Gamma radiation from PSR B1055-52

Abstract

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