Transition Probability (TP) References to Original Literature: C


Carbon, Z=6

Return to: Transition Probability References


C I (TP) Allowed

  1. Luo, D. and Pradhan, A. K. (1989), J. Phys. B 22, 3377.
  2. Hibbert, A., Biemont, E., Godefroid, M., and Vaeck, N. (1993), Astron. Astrophys., Suppl. Ser. 99, 179.
  3. Nussbaumer, H. and Storey, P. J. (1984), Astron. Astrophys. 140, 383.
  4. Weiss, A. W., private communication.
  5. Goldbach, C. and Nollez, G. (1987), Astron. Astrophys. 181, 203.
  6. Goldbach, C., Martin, M., and Nollez, G. (1989), Astron. Astrophys. 221, 155.
  7. Jones, D. W. and Wiese, W. L, (1984), Phys. Rev. A 29, 2597.
  8. Musielok, J., Veres, G., and Wiese, W. L, J. Quant. Spectrosc. Radiat. Transfer 57, 395 (1997).
  9. Haar, R. R., Curtis, L. J., Kvale, T. J., Beideck, D. J., Martinson, I., and Hellborg, R. (1991), Astron. Astrophys. 241, 321.

C I (TP) Forbidden

  1. Hibbert, A., Biemont, E., Godefroid, M., and Vaeck, N. (1993), Astron. Astrophys. Suppl. Ser. 99, 179.
  2. Froese Fischer, C. and Saha, H. P. (1985), Phys. Scr. 32, 181.
  3. Shortley, G. H., Allen, L. H., Baker, J. G., and Menzel, D. H. (1941) Astrophys. J. 93, 17.

C II (TP) Allowed

  1. Lennon, D. J., Dufton, P. L., Hibbert, A., and Kingston, A. E. (1985), Astrophys. J. 294, 200.
  2. Yu Yan,Taylor, K. T., and Seaton, M. J. (1987), J. Phys. B 20, 6399.
  3. Fang, Z., Kwong, V. H. S., Wang, J., and Parkinson, W. H. (1993), Phys. Rev. A 48, 1114.
  4. Nussbaumer, H. and Storey, P. J. (1981), Astron. Astrophys. 96, 91.
  5. Reistad, N., Hutton, R., Nilsson, A. E., Martinson, I., and Mannervik, S. (1986), Phys. Scr. 34, 151.
  6. Goly, A. and Weniger, S. (1982), J. Quant. Spectrosc. Radiat. Transfer 28, 389.
  7. Glenzer,S., Kunze, H.-J., Musielok, J., Kim, Y.-K., and Wiese, W. L. (1994), Phys. Rev. A 49, 221.
  8. Huber, M. C. E., Sandeman, R. J., and Tozzi, G. P. (1984), Phys. Scr. T8, 95.
  9. Baudinet-Robinet,Y., Dumont, P.-D., Garnir, H.-P., and El Hindy, A. (1989), Phys. Rev. A 40, 6321.
  10. Weiss, A. W., private communication.

C II (TP) Forbidden

  1. Froese Fischer, C. (1983), J. Phys. B 16, 157.

C III (TP) Allowed

  1. Weiss, A. W., private communication.
  2. Tully, J. A., Seaton M. J., and Berrington, K. A. (1990), J. Phys. B 23, 3811.
  3. Hibbert, A. (1976), J. Phys. B 9, 2805.
  4. Allard, N., Artru, M.-C., Lanz, T., and LeDorneuf, M. (1990) (1991), Astron. Astrophys., Suppl. Ser. 84, 563 and 91, 399 .
  5. Kwong,V. H. S., Fang, Z., Gibbons, T. T., Parkinson, W. H., and Smith, P. L. (1993), Astrosphys. J. 411. 431.
  6. Hibbert, A. (1980), J. Phys. B 13, 1721.
  7. Reistad, N., Hutton, R., Nilson, A. E., Martinson, I., and Mannervik, S. (1986), Phys. Scr. 34, 151.
  8. Baudinet-Robinet, Y., Dumont, P.-D., Garnir, H.-P., and El Hindy, A. (1989), Phys. Rev. A 40, 6321.

C III (TP) Forbidden

  1. Glass, R. (1982), Astrophys. Space Sci. 87, 41.
  2. Glass, R. (1983), Astrophys. Space Sci. 91, 417.
  3. Glass, R. (1983), Astrophys. Space Sci. 92, 307.
  4. Nussbaumer, H. and Storey, P. J. (1978), Astron. Astrophys. 64, 139.
  5. Pasternak, S. (1940), Astrophys. J. 92, 129.

C IV (TP) Allowed

  1. Peach, G., Saraph, H. E., and Seaton, M. J. (1988), J. Phys. B 21, 3669.
  2. Bi‚mont, E. (1977), Astron. Astrophys., Suppl. Ser. 27, 489.
  3. Lindgard, A. and Nielsen, S. E. (1977) At. Data Nucl. Data Tables 19, 533.
  4. Martin, G. A. and Wiese,W. L. (1976), J. Phys. Chem. Ref. Data 5, 537.
  5. Baudinet-Robinet, Y., Dumont, P.-D., Garnir, H.-P., and El Himdy, A. (1989), Phys. Rev. A 40, 6321.
  6. Laughlin, C. (1988), Z. Phys. D 9, 273.
  7. Blanke, J. H., Heckmann, P. H., and Träbert, E. (1985), Phys. Scr. 32, 509.
  8. Davis, B. F. and Chung, K. T. (1988), Phys. Rev. A 37, 111.

C V (TP)

  1. Cann, N. M. and Thakkar, A. J. (1992), Phys. Rev. A 46, 5397.
  2. Schiff, B. and Pekeris, C. L. (1964), Phys. Rev. 134, A638.
  3. Kono, A. and Hattori, S. (1984), Phys. Rev. A 30, 2093.
  4. Fernley, J. A.,Taylor, K. T., and Seaton, M. J. (1987), J. Phys. B 20, 6457.
  5. Kim, Y.-K. and Weiss, A. W. (1993), private communication.

C V (TP) Forbidden

  1. Drake, G. W. F. (1971), Phys. Rev. A 3, 908.
  2. Schmidt, H. T. P., Forck, Grieser, M., Habs, D., Kenntner, J., Miersch, G., Repnow, R., Schramm, U., Schüssller, T., Schwalm,D., and Wolf, A. (1994), Phys. Rev. Lett. 72, 1616.
  3. Drake, G. W. F. (1969), Astrophys. J. 158, 1199.
  4. Kundu,B., Mukherjee, P. K., and Roy, H. P. (1989), Phys. Scr. 39, 722.
  5. Godefroid, M. and Verhaegen, G. (1980), J. Phys. B. 13, 3081.

C VI (TP) Allowed

  1. Corney, A. (1977), Atomic and Laser Spectroscopy, Oxford Univ. Press, Oxford.
  2. Erickson, G. W. (1977), J. Phys. Chem. Ref. Data 6, 831.
  3. Johnson, W. R. and Soff, G. (1985), At. Data Nucl. Data Tables 33, 405.

Return to: Transition Probability References