Abstract
THE nature of gamma-ray-burst (GRB) sources has remained a mystery, in part because of the lack of any optical identification. Recently, deep CCD photometry has identified the optical counterpart G″ to the γ-ray source Geminga, whose location on a colour-magnitude diagram is unique1. Although the X-rays from G″ are probably due to thermal emission from the neutron star, the implied column density (≳ 5 x 1020) is inconsistent with the distance (D < 100 pc) required to fit the optical flux to the same spectral component. Here I show that the optical emission could be due instead to a cold accretion disk with accretion rate Ṁ ≈ 1011 g s−1. This has promising implications for the search for the optical counterparts to GRB sources whose basic physical parameters may resemble those of radio pulsars and related objects such as Geminga. I argue that a similar search in the field of a GRB location should produce candidates similar to G″ if 20 pc ≲ DGRB ≲ 500 pc, as predicted by the disk-reprocessing model for the associated optical transients. This possibility is discussed in the light of the fact that the first optical counterpart to a GRB source may already have been found, which, if it is confirmed, may be used to test the accretion-disk model.
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References
Halpern, J. P. & Tytler, D. Astrophys. J. 330, 201–217 (1988).
Liang, E. P. & Petrosian, V. AIP Conf. Proc. (AIP, New York, 1986).
Mazets, E. P. et al. Nature 290, 378–380 (1981).
Hueter, G. J. High Energy Transients in Astrophysics (ed. Woosley, S. E.) 373–377 (AIP, New York, 1984).
Murakami, T. et al. Nature 335, 234–235 (1988).
Melia, F. Astrophys. J. 334, L9–L12 (1988).
Melia, F. Nature 336, 658–660 (1988).
Fenimore, E. E. et al. Astrophys. J. (submitted).
Helfand, D. J. & Vrtilek, S. D. Nature 304, 41–43 (1983).
Michel, F. C. Astrophys. J. 290, 721–727 (1985).
Katz, J. I. Astrophys. Lett. 24, 183 (1985).
Ruderman, M. A. 13th Texas Symp. on Relativistic Astrophysics (ed. Ulmer, M. P.) 448–459 (World Scientific, Singapore, 1987).
Schaefer, B. E. Adv. Space Res. 6, 47 (1987).
Melia, F. Astrophys. J. 324, L21–L25 (1988).
Smith, F. G. Pulsars (Cambridge Univ. Press, 1977).
Matz, S. M. et al. Astrophys. J. 288, L37–L40 (1985).
Kouveliotou, C. Astrophys. J. 330, L101–L105 (1988).
Manchester, R. N. & Taylor, J. H. Pulsars (Freeman, San Francisco, 1977).
Melia, F. Astrophys. J. 335, 965–970 (1988).
Bignami, G. F. et al. Astrophys. J. 319, 358–361 (1987).
Romani, R. Astrophys. J. (in the press).
Michel, F. C. & Dessler, A. J. Astrophys. J. 251, 654–664 (1981).
Kafka, P. & Meyer, F. High Energy Transients in Astrophysics (ed. Woosley, S. E.) 578–580 (AIP, New York, 1984).
Epstein, R. I. Astrophys. J. 291, 822–833 (1985).
Melia, F., Rappaport, S. & Joss, P. C. Astrophys. J. 305, L51–L55 (1986).
Melia, F. Proc. Sofia COSPAR Symp. (ed. White, N.) 641–652 (1988).
Helfand, D. J. et al. Nature 283, 337–343 (1980).
Schaefer, B. E. Nature 302, 43–45 (1981).
Pedersen, H. et al. Astrophys. J. 270, L43–L47 (1983).
Schaefer, B. E. et al. Astrophys. J. 270, L49–L52 (1983).
Boer, M. et al. Astr. Astrophys. 202, 117–123 (1988).
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Melia, F. Geminga and the search for optical counterparts of γ-ray-burst sources. Nature 338, 322–324 (1989). https://doi.org/10.1038/338322a0
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DOI: https://doi.org/10.1038/338322a0
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