Abstract
Given that pulsars and AGN are the only identified GeV point sources, it isn’t too bold to infer a substantial pulsar contribution to the Unidentified population. Specific models however predict differently the types of pulsars present in the observed sample. The dominant factors are the efficiency of spindown-gamma conversion, the high energy beam shape and the gamma ray spectrum. I’ll review briefly the main features of the `outer gap’ picture. Consequences for the relative numbers and Galactic distributions of the objects expected in the EGRET survey are then discussed, including young pulsars, `Geminga’s, binaries and millisecond pulsars. With recent counterpart work, we can already test and refine these predictions. The final, and main, point is that what we actually see teaches us in return important lessons about the pulsar physics. With up to a third of the spindown luminosity appearing as GeV gamma rays, these lessons give powerful constraints on the nature of the pulsar machine
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Becker, W. & Truemper, J 1999,x AA, 341, 803
Brazier, K.T.S., Reimer, 0., Kanbach, G. & Carramiñana, A. 1998, MNRaS, 295, 819
Cheng, K.S., Ho. C. & Ruderman, M.A. 1986, x ApJ, 300, 522 Cheng, K.S., Ruderman, M. A. & Zhang, L. 2000, x ApJ, 537, 964
Cordes, J.M & Chernoff, D. F. 1997, x ApJ, 482, 971
Cusumano, G. et al 2000, x ApJ, 528, L25
Daugherty, J.K. & Harding, A.K. 1996, x ApJ, 458, 278
de Jager, O.C. et al. 1996, x ApJ, 457 253
Gehrels, N., et al 2000, x Nature, 404, 363
Gosset, E. 1987, x AA, 188, 258
Grenier, I.A. & Perrot, C. 1999 in Proc. x XXVI Int’l Cosmic Ray Conf, 3, 476
Harding, A.K. & Musslimov, A.G. 1998, x ApJ 508 328
Harding, A.K. & Zhang, B. 2001, ApJ in press
Hirotani, K. 2000, x MNRaS,317, 225
Holloway, N.J. 1973, x Nature, 246, 6
Iben, I., Tutukov, A.V. & Yungelson, L.R. 1995, x ApJS, 100, 217
Kaaret, P., Cusumano, G. & Sacco, B. 2000, x ApJ, 542, L41 Kaaret, P. & Cottam, J. 1996, xApJ, 462, L35
Kaspi, V. M. et al. 2000, x ApJ, 528, 445
Kuiper, L. et al. 2000, x AA, 359 615
Lyne, A.G, Si Graham-Smith, F. 1998 x Pulsar Astronomy (Cambridge:Cambrid McLaughlin, M.A., et al 1996, ApJ, 473, 763
Merck, M. et al. 1996, x AASupl, 120465
Michelson, P.F., et al. 1994, x ApJ, 435218
Mirabel, N. & Halpern, J.P. 2001, x ApJ, 547, L137
Poeppel, W.G.L. 1997. x Fund. Cos. phys., 18, 1
Ramanamurthy, P.V., et al. 1996, x ApJ, 458, 755
Romani, R.W. 1996, x ApJ, 470, 469
Romani, R.W. & Yadigaroglu 1995, x ApJ, 438,314 (RY95)
Tompkins, W. 1999, PhD Thesis, Stanford University
Yadigaroglu, I.-A. & Romani, R.W. 1997, x ApJ, 476, 347
(YR97)
Zhang, B. & Harding, A.K. 2000, x ApJ 532, 1150
Zhang, L., Zhang, Y.J. and Cheng, K.S. 2000, x AA, 357 957
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2001 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Romani, R.W. (2001). Gamma-Ray Pulsars in the Unidentified Population: The ‘Outer Gap’ Perspective. In: Carramiñana, A., Reimer, O., Thompson, D.J. (eds) The Nature of Unidentified Galactic High-Energy Gamma-Ray Sources. Astrophysics and Space Science Library, vol 267. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1007-8_11
Download citation
DOI: https://doi.org/10.1007/978-94-010-1007-8_11
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3875-1
Online ISBN: 978-94-010-1007-8
eBook Packages: Springer Book Archive