Abstract
The discovery of the microlensing effect has found out the new population — dark bodies having mass of the order of 0.1M ⊙ which form the halo of our Galaxy. There are two main criteria which identify a light curve as the reveal of the microlensing effect. They are symmetry of the light curve and equal amplification in different colors. We consider polarization of the light beam arising in microlensing effect and find that additional test is possible — polarization of light in the case of a finite star disk. Consequences of polarization are also considered.
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Alcock, C., Akerlof, C.W., Allsman, R.A.et al.: 1993,Nature 365, 621.
Aubourg, E., Bareyre, P., Brehin, S.et al.: 1993,Nature 365, 623.
Barnes, T.G., Evans, D.S. and Moffett, T.J.: 1978,Monthly Notices Roy. Astron. Soc. 183, 285.
Blair, D.G. and Sazhin, M.V.: 1993,Astron. Astrophys. Trans. 3, 191.
Bochkarev, N.G. and Karitskaya, E.A.: 1983,Soviet Astron. Letters 9, 14.
Bochkarev, N.G., Karitskaya, E.A. and Sakhibullin, N.A.: 1985,Astrophys. Space Sci. 108, 15.
Bogdanov, M.B.: 1988,Astron. Circ. N1526, 10.
Bogdanov, M.B.: 1987,Astron. Zh. 64, 1300.
Bogdanov, M.B. and Cherepashchuk, A.M.: 1995,Astron. Zh. 72, N6.
Bildhauer, S.: 1989,Astron. Astrophys. 219, 25.
Byalko, A.V.: 1969,Soviet Astron. 46, 998.
Cassinelli, J.P. and Hummer, D.G.: 1971,Monthly Notices Roy. Astron. Soc. 153, 9.
Cassinelli, J.P. and Hoffman, N.M.: 1975,Monthly Notices Roy. Astron. Soc. 173, 789.
Chandrasekhar, S.: 1953,Radiative Transfer, Dover Publ.
Cherepaschuk, A.M., Sazhin, M.V. and Trifalenkov, I.A.: 1995,Astrophys. Space Sci. 229, 265.
Eaton, J.A. and Poe, C.H.: 1984,Acta Astron. 34, 97.
Griest, K.: 1991,Astrophys. J. 366, 412.
Labeyrie, A.: 1994,Astron. Astrophys. 284, 689.
Liebes, R.: 1964,Phys. Rev. B133, 835.
Mashoon, B.: 1975,Phys. Rev. 11, 2679.
McBreen, B. and Metcalfe, L.: 1987,Nature 330, 348.
Nagirner, D.I.: 1962,Proc. Astron. Obs. of LSU 19, 79.
Paczinsky, B.: 1986,Astrophys. J. 304, 1.
Refsdal, S.: 1964,Monthly Notices Roy. Astron. Soc. 128, N4.
Sams, D.C. and Johnston, I.D.S.: 1974,Monthly Notices Roy. Astron. Soc. 168, 463.
Sazhin, M.V.: 1987,Astron. Circular, N1500.
Sazhin, M.V. and Cherepashchuk, A.M.: 1994,Astron. J. Letters 20, 523.
Sazhin, M.V. and Cherepashchuk, A.M.: 1995,Astron. J. Letters 21, 230.
Schneider, P. and Wagoner, R.V.: 1987,Astrophys. J. 314, 154.
Simmons, J.F.L., Willis, J.P. and Newsam, A.M.: 1995,Astron. Astrophys. 293, L46.
Sobolev, V.V.: 1956,Radiative transfer in stellar and planetary atmospheres, Moscow, GOSTEKHIZDAT (in russian).
Spiro, M.: 1990, in: K.K. Phua and Y. Yamaguchi (eds.),Proc. of 25th Intern. Conf. on High Energy Phys., Vol.II, p. 463.
Udalski, A., Szymanski, M., Kaluzny, J., Kubiak, M., Mateo, M. and Krzeminsky, W.: 1994,Astrophys. J. Letters 426, L69.
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Bogdanov, M.B., Cherepashchuk, A.M. & Sazhin, M.V. Microlensing and polarization. Astrophys Space Sci 235, 219–231 (1996). https://doi.org/10.1007/BF00644442
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DOI: https://doi.org/10.1007/BF00644442