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Referencias:

• Spielberger, L., Jagutzki, O., Dörner, R., Ullrich, J., Meyer, U., Mergel, V., Unverzagt, M., Schmidt-Böcking, H., (1995) Phys. Rev. Lett., 74, p. 4615. , PRLTAO
• Spielberger, L., Jagutzki, O., Krässig, B., Meyer, U., Khayyat, K., Mergel, V., Tschentscher, T., Schmidt-Böcking, H., (1996) Phys. Rev. Lett., 76, p. 4685. , PRLTAO
• Wehlitz, R., Hentges, R., Prümper, G., Farhat, A., Buslaps, T., Berrah, N., Levin, J.C., Becker, U., (1996) Phys. Rev. A, 53, p. R3720. , PLRAAN
• Levin, J.C., Bradley Armen, G., Sellin, I.A., (1996) Phys. Rev. Lett., 76, p. 1220. , PRLTAO
• Sagurton, M., Bartlett, R.J., Samson, J.A.R., He, Z.H., Morgan, D., (1995) Phys. Rev. A, 52, p. 2829. , PLRAAN
• Surić, T., Pisk, K., Logan, B.A., Pratt, R.H., (1994) Phys. Rev. Lett., 73, p. 790. , PRLTAO
• Andersson, L.R., Burgdörfer, J., (1994) Phys. Rev. A, 50, p. R2810. , PLRAAN
• Kornberg, M.A., Miraglia, J.E., (1996) Phys. Rev. A, 53, p. R3709. , PLRAAN
• Bergstrom, P.M., Jr., Hino, K., Macek, J.H., (1995) Phys. Rev. A, 51, p. 3044. , PLRAAN
• Amusia, M.Y., Mikhailov, A.I., (1995) J. Phys. B, 28, p. 1723. , JPAPEH
• Eisenberger, P., Platzman, P.M., (1970) Phys. Rev. A, 2, p. 415. , PLRAAN
• Bloch, B.J., Mendelsohn, L.B., (1974) Phys. Rev. A, 9, p. 129. , PLRAAN
• Kornberg, M.A., Miraglia, J.E., (1993) Phys. Rev. A, 48, p. 3714. , PLRAAN
• Hino, K., (1993) Phys. Rev. A, 47, p. 4845. , PLRAAN
• Bergstrom, P.M., Jr., Surić, T., Pisk, K., Pratt, R.H., (1993) Phys. Rev. A, 48, p. 1134. , PLRAAN
• Weiss, A.W., (1961) Phys. Rev., 122, p. 1826. , PHRVAO
• If both orbitals are described by the same charge (Formula presented) the profile is of the form (Formula presented); whereas if both orbitals have different charges (Formula presented) it is of the form (Formula presented); Wong, T.C., Mendelsohn, L.B., Grossman, H., Wellenstein, H.F., (1982) Phys. Rev. A, 26, p. 181. , PLRAAN
• It should be pointed out that the sign of the asymmetry, as defined by Eq. (17), depends on how one defines (Formula presented) If instead of defining (Formula presented) as in Eq. (7), we define (Formula presented), the asymmetry will change sign; At the photon energies considered in Fig. 11, the total electron energies at the peak value (Formula presented) are about 3.2 keV and 5.4 keV for (Formula presented) keV and (Formula presented) keV, respectively. The main contribution to the profile (Formula presented) comes here from an asymmetric electron energy sharing, in which one of both electrons takes less than 50 eV. This gives a relative momentum (Formula presented) a.u., and thus the electron-electron Sommerfeld parameter is (Formula presented) a.u. Final-state correlations are then expected to play a minor role in this case. For high-energy photoionization, where a similar asymmetric energy sharing takes place, the use of Eq. (5) for describing the final state gives good agreement with the experiments; Surić, T., Pisk, K., Pratt, R.H., (1996) Phys. Lett. A, 211, p. 289. , PYLAAG
• Dalgarno, A., Sadeghpour, H.R., (1992) Phys. Rev. A, 46, p. R3591. , PLRAAN
• Forrey, R.C., Sadeghpour, H.R., Baker, J.D., Morgan, J.D., III, Dalgarno, A., (1995), 51, p. 2112; Wang, J., McGuire, J.H., Burgdörfer, J., Qiu, Y., (1996) Phys. Rev. Lett., 77, p. 1723. , PRLTAO
• Ullrich, J., Moshammer, R., Dörner, R., Jagutzki, O., Mergel, V., Schmidt-Böcking, H., Spielberger, L., (1997) J. Phys. B, 30, p. 2917. , JPAPEH
• Dörner, R., Feagin, J.M., Cocke, C.L., Bräuning, H., Jagutzki, O., Jung, M., Kanter, E.P., Vogt, T., (1996) Phys. Rev. Lett., 77, p. 1024. , PRLTAO

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