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Some Constraints on Neutron Star Properties from Gamma Ray Burster Observations

Published online by Cambridge University Press:  04 August 2017

K. Hurley
K. Hurley*
Affiliation:
Centre d'Etude Spatiale des Rayonnements (CNRS-UPS), B.P. 4346, 31029 Toulouse Cedex, France

Abstract

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The results of recent soft X-ray and optical searches for quiescent gamma ray burster counterparts are used to constrain the properties of the neutron stars responsible for bursters. Ages are restricted to the range 2×105 y and above based on temperature upper limits and theoretical cooling curves, or 107 y and above if bursters have evolved from pulsars. Velocities are greater than 20 km/s if the neutron stars are unmagnetized. Practically no main sequence star could have escaped detection in the optical/IR searches, so if the neutron stars are in binary systems, the companion is most likely a degenerate, low mass, low temperature object.

Type
VI. Other Manifestations of Neutron Stars and Their Place in Neutron Star Evolution
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 489 - 500
Copyright
Copyright © Reidel 1987 

References

Allen, C. 1976, Astrophysical Quantities, Athlone Press, London.Google Scholar
Apparao, K., and Allen, D. 1982, Astron. Astrophys. Lett. 107, L5.Google Scholar
Atteia, J.-L., Boer, M., Hurley, K., Niel, M., Chevalier, C., Ilovaisky, S., Motch, C., Taylor, B., Sims, M., Pizzichini, G., Mason, K., Branduardi-Raymont, G., Cordova, F., Evans, W., Klebesadel, R., Laros, J., and Martin, C. 1986a, XXVI COSPAR Topical Meeting E.4 on Gamma Ray Bursts, and New Results on Gamma Radiation from the Galaxy, Toulouse, France, to be published in Adv. Space Res. Google Scholar
Atteia, J.-L., Barat, C., Hurley, K., Niel, M., Vedrenne, G., Evans, W., Fenimore, E., Klebesadel, R., Laros, J., Cline, T., Desai, U., Teegarden, B., Estulin, I., Zenchenko, V., Kuznetsov, A., and Kurt, V. 1986b, Ap. J. (submitted).Google Scholar
Bancall, J. 1984, Ap. J. 276, 169.Google Scholar
Barat, C., Chambon, G., Hurley, K., Niel, M., Vedrenne, G., Estuline, I., Kurt, V., and Zenchenko, V. 1979, Astron. Astrophys. Lett. 79, L24.Google Scholar
Barat, C., Hurley, K., Niel, M., Vedrenne, G., Cline, T., Desai, U., Schaefer, B., Teegarden, B., Evans, W., Fenimore, E., Klebesadel, R., Laros, J., Estulin, I., Zenchenko, V., Kuznetsov, A., Kurt, V., Ilovaisky, S., and Motch, C. 1984, Ap. J. Lett. 286, L5.Google Scholar
Bignami, G. 1985, Proc. NATO Advanced Study Institute on High Energy Phenomena Around Collapsed Stars, Cargese, Corsica, D. Reidel Pub. Co., Dordrecht, Holland.Google Scholar
Bussard, R. and Lamb, F. 1982, in Gamma Ray Transients and Related Astrophysical Phenomena, Eds. Lingenfelter, R., Hudson, H., and Worrall, D., AIP Conference Proc. No. 77, AIP Press, New York, p. 189.Google Scholar
Chevalier, C., Ilovaisky, S., Motch, C., Barat, C., Hurley, K., Niel, M., Vedrenne, G., Laros, J., Evans, D., Fenimore, E., Klebesadel, R., Estulin, I., and Zenchenko, V. 1981, Astron. Astrophys. Lett. 100, L1.Google Scholar
Davies, R., and Pringle, J. 1981, Mon. Not. R. astr. Soc. 196, 209.Google Scholar
Dennis, B., Frost, K., Kiplinger, A., Orwig, L., Desai, U., and Cline, T. 1982, in Gamma Ray Transients and Related Astrophysical Phenomena, Eds. Lingenfelter, R., Hudson, H., and Worrall, D., AIP Conference Proceedings No. 77, AIP Press, New York, p. 153.Google Scholar
Epstein, R. 1985, Ap. J. 297, 555.Google Scholar
Fenimore, E., Klebesadel, R., and Laros, J. 1983, Adv. Space Res. 3(4), 207.CrossRefGoogle Scholar
Fenimore, E., Klebesadel, R., Laros, J., Stockdale, R., and Kane, S. 1982, Nature 297, 665.CrossRefGoogle Scholar
Glen, G. and Sutherland, P. 1980, Ap. J. 239, 671.Google Scholar
Hameury, J.-M. 1984, , Universite de Paris VII Helfand, D. 1985, Proc. NATO Advanced Study Institute on High Energy Phenomena Around Collapsed Stars, Cargese, Corsica, D. Reidel Pub. Co., Dordrecht, Holland.Google Scholar
Higdon, J. and Lingenfelter, R. 1984, in High Energy Transients in Astrophysics, Ed. Woosley, S., AIP Conf. Proc. No. 115, AIP Press, N.Y., p. 568.Google Scholar
Hueter, G. 1984, in High Energy Transients in Astrophysics, Ed. Woosley, S., AIP Conference Proceedings No. 115, AIP Press, N.Y., p. 373.Google Scholar
Hurley, K. 1985, Proc. NATO Advanced Study Institute on High Energy Phenomena Around Collapsed Stars, Cargese, Corsica, D. Reidel Pub. Co., Dordrecht, Holland.Google Scholar
Illarionov, A. and Sunyaev, R. 1975, Astron. Astrophys. 39, 185.Google Scholar
Lamb, D. 1985, Proc. NATO Advanced Study Institute on High Energy Phenomena Around Collapsed Stars, Cargese, Corsica, D. Reidel Pub. Co., Dordrecht, Holland.Google Scholar
Lamb, F. 1985, ibid.Google Scholar
Lasota, J. and Belli, B. 1983, Nature 304, 139.CrossRefGoogle Scholar
Liang, E. 1985, UCRL Preprint 93454, Lawrence Livermore Nat'l. Lab.Google Scholar
Liang, E. and Petrosian, V. 1986, Gamma Ray Bursts, AIP Conf. Proc. No. 141, AIP Press, New York.Google Scholar
Lyne, A., Manchester, R., and Taylor, J. 1985, Mon. Not. R. astr. Soc. 213, 613.CrossRefGoogle Scholar
Mazets, E., Golenetskii, S., Aptekar, R., Gur'yan, Yu., and Il'inskii, V. 1981a, Nature 290, 378.Google Scholar
Mazets, E., Golenetskii, S., Il'inskii, V., Panov, V., Aptekar, R., Gur'yan, Yu., Proskura, M., Sokolov, I., Sokolova, Z., Kharitonova, T., Dyatchkov, A., and Khavenson, N. 1981b, Astrophys. and Space Sci. 80, 3.Google Scholar
Motch, C., Pedersen, H., Ilovaisky, S., Chevalier, C., Hurley, K., and Pizzichini, G. 1985, Astron. Astrophys. 145, 201.Google Scholar
Pedersen, H., Motch, C., Tarenghi, M., Danziger, J., Pizzichini, G., and Lewin, W. 1983, Ap. J. Lett. 270, L43.Google Scholar
Peng, Q., Huang, K., and Huang, J. 1982, Astron. Astrophys. 107, 258.Google Scholar
Pizzichini, G., Gottardi, M., Atteia, J.-L., Barat, C., Hurley, K., Niel, M., Vedrenne, G., Laros, J., Evans, W., Fenimore, E., Klebesadel, R., Cline, T., Desai, U., Kurt, V., Kuznetsov, A., and Zenchencko, V. 1986, Ap. J. 301, 641.CrossRefGoogle Scholar
Rappaport, S. and Joss, P. 1985, Nature 314, 242.Google Scholar
Schaefer, B., and Ricker, G. 1983, Nature 302, 43.Google Scholar
Schaefer, B., Seitzer, P., and Bradt, H. 1983, Ap. J. Lett. 270, L49.Google Scholar
Schaefer, B., and Cline, T. 1985, Ap. J. 289, 490.Google Scholar
Schaefer, B., Cline, T., Desai, U., Teegarden, B., Atteia, J.-L., Barat, C., Hurley, K., Niel, M., Evans, W., Fenimore, E., Klebesadel, R., Laros, J., Estulin, I., and Kuznetsov, A. 1986, Ap. J. (submitted).Google Scholar
Shklovskii, I. and Mitrofanov, I. 1985, Mon. Not. R. astr. Soc. 212, 545.Google Scholar
Trümper, J. 1982, in Gamma Ray Transients and Related Astrophysical Phenomena, Eds. Lingenfelter, R., Hudson, H., and Worrall, D., AIP Conference Proceedings No. 77, AIP Press, New York, p. 179.Google Scholar
Trümper, J. 1985, Proc. NATO Advanced Study Institute on High Energy Phenomena Around Collapsed Stars, Cargese, Corsica, D. Reidel Pub. Co., Dordrecht, Holland.Google Scholar
Trumper, J. 1986, in Cosmic Radiation in Contemporary Astrophysics, Ed. Shapiro, M., D. Reidel Publishing Co., Dordrecht, Holland, p. 217.Google Scholar
Ventura, J., Bonazzola, S., Hameury, J., and Heyvaerts, J. 1983, Nature 301, 491.CrossRefGoogle Scholar
Wood, K., Byram, E., Chubb, T., Friedman, H., Meekins, J., Share, G., and Yentis, D. 1981, Ap. J. 247, 642.Google Scholar
Wood, K., Meekins, J., Yentis, D., Smathers, H., McNutt, D., Bleach, R., Byram, E., Chubb, T., Friedman, H., and Meidav, M. 1984, Ap. J. Supp. 56, 507.Google Scholar