Be+ 1 4 2 146883.(1S) 1 1s22s(2S) (2)0( 0.5) 0. 2 1s22p(2P) (2)1( 2.5) 31933. 3 1s23s(2S) (2)0( 0.5) 88232. 4 1s23p(2P) (2)1( 2.5) 96497. 5 1s23d(2D) (2)2( 4.5) 98055. 6 1s24s(2S) (2)0( 0.5) 115464. 7 1s24p(2P) (2)1( 2.5) 118761. 8 1s24d(2D) (2)2( 4.5) 119421. 9 1s24f(2F) (2)3( 6.5) 119447. -1 2.00 3 2.00+03 5.00+03 1.00+04 2.00+04 5.00+04 1.00+05 2.00+05 5.00+05 1.00+06 2 1 1.14+08 1.32+01 1.36+01 1.43+01 1.57+01 1.90+01 2.30+01 2.88+01 3.91+01 4.80+01 1.39+01 3 1 0.00+00 1.56+00 1.45+00 1.29+00 1.11+00 9.49-01 9.18-01 9.59-01 1.08+00 1.19+00 1.54+00 4 1 1.65+08 7.64-01 6.71-01 6.23-01 5.73-01 4.94-01 4.53-01 4.57-01 5.81-01 7.85-01 7.26-01 5 1 0.00+00 7.09-01 7.72-01 8.34-01 8.90-01 9.87-01 1.14+00 1.40+00 1.90+00 2.29+00 3.32+00 6 1 0.00+00 2.80-01 2.63-01 2.33-01 2.02-01 1.76-01 1.72-01 1.82-01 2.08-01 2.30-01 3.06-01 7 1 9.48+07 2.23-01 2.17-01 2.06-01 1.89-01 1.66-01 1.55-01 1.55-01 1.90-01 2.49-01 2.23-01 8 1 0.00+00 1.83-01 1.90-01 1.91-01 1.91-01 2.04-01 2.32-01 2.84-01 3.88-01 4.78-01 7.55-01 9 1 0.00+00 1.63-01 1.78-01 1.73-01 1.58-01 1.40-01 1.35-01 1.38-01 1.46-01 1.48-01 1.27-01 3 2 4.15+08 4.88+00 4.68+00 3.92+00 3.03+00 2.22+00 2.09+00 2.43+00 3.62+00 4.95+00 3.06+00 4 2 0.00+00 7.40+00 6.37+00 5.85+00 5.38+00 4.82+00 4.62+00 4.74+00 5.35+00 5.97+00 8.11+00 5 2 1.12+09 6.63+00 7.08+00 7.67+00 8.46+00 1.03+01 1.34+01 1.90+01 3.11+01 4.32+01 2.55+01 6 2 1.44+08 1.01+00 8.78-01 7.30-01 5.85-01 4.42-01 3.91-01 3.95-01 4.85-01 6.04-01 3.24-01 7 2 0.00+00 1.87+00 1.73+00 1.58+00 1.41+00 1.19+00 1.07+00 1.03+00 1.08+00 1.18+00 1.59+00 8 2 3.80+08 1.47+00 1.51+00 1.55+00 1.60+00 1.86+00 2.33+00 3.19+00 5.02+00 6.81+00 3.73+00 9 2 0.00+00 1.26+00 1.39+00 1.37+00 1.28+00 1.19+00 1.21+00 1.31+00 1.51+00 1.63+00 1.82+00 4 3 1.26+07 4.28+01 4.47+01 5.29+01 6.97+01 1.10+02 1.56+02 2.15+02 3.07+02 3.79+02 8.84+01 5 3 0.00+00 2.35+01 2.45+01 2.47+01 2.42+01 2.29+01 2.24+01 2.27+01 2.39+01 2.47+01 2.57+01 6 3 0.00+00 5.56+00 5.02+00 4.38+00 3.88+00 3.73+00 4.09+00 4.73+00 5.76+00 6.47+00 8.13+00 7 3 1.36+07 2.66+00 2.39+00 2.20+00 1.99+00 1.81+00 1.81+00 2.03+00 2.72+00 3.54+00 1.89+00 8 3 0.00+00 2.43+00 2.58+00 2.66+00 2.77+00 3.20+00 3.87+00 4.74+00 5.76+00 6.22+00 6.47+00 9 3 0.00+00 3.28+00 3.69+00 3.84+00 3.95+00 4.43+00 5.13+00 5.98+00 6.86+00 7.20+00 7.25+00 5 4 7.89+04 2.67+02 3.03+02 3.48+02 4.11+02 5.22+02 6.26+02 7.46+02 9.15+02 1.04+03 1.37+02 6 4 9.84+07 8.81+00 7.84+00 6.52+00 5.76+00 6.75+00 9.89+00 1.58+01 2.79+01 3.90+01 1.90+01 7 4 0.00+00 1.27+01 1.15+01 1.11+01 1.13+01 1.33+01 1.64+01 2.03+01 2.57+01 2.94+01 3.85+01 8 4 1.09+08 1.42+01 1.47+01 1.49+01 1.53+01 1.94+01 2.84+01 4.56+01 8.10+01 1.14+02 5.96+01 9 4 0.00+00 1.21+01 1.39+01 1.49+01 1.64+01 2.15+01 2.92+01 3.97+01 5.37+01 6.15+01 7.24+01 6 5 0.00+00 1.59+01 1.31+01 9.77+00 6.87+00 4.57+00 3.89+00 3.81+00 4.01+00 4.12+00 3.99+00 7 5 8.83+06 2.39+01 1.93+01 1.64+01 1.36+01 1.08+01 9.57+00 9.26+00 1.02+01 1.17+01 3.93+00 8 5 0.00+00 2.40+01 2.40+01 2.33+01 2.27+01 2.44+01 2.83+01 3.35+01 4.06+01 4.50+01 5.42+01 9 5 2.22+08 4.27+01 5.02+01 5.58+01 6.46+01 9.33+01 1.41+02 2.22+02 3.75+02 5.08+02 2.09+02 7 6 2.74+06 5.27+01 7.44+01 1.18+02 1.99+02 3.86+02 5.92+02 8.46+02 1.21+03 1.48+03 3.02+02 8 6 0.00+00 6.56+01 7.24+01 7.70+01 8.14+01 8.77+01 9.35+01 9.94+01 1.05+02 1.07+02 1.07+02 9 6 0.00+00 2.97+01 2.81+01 2.53+01 2.17+01 1.79+01 1.66+01 1.64+01 1.67+01 1.69+01 1.67+01 8 7 2.55+04 6.81+02 8.99+02 1.17+03 1.55+03 2.18+03 2.75+03 3.35+03 4.14+03 4.69+03 5.82+02 9 7 0.00+00 1.37+02 1.48+02 1.48+02 1.40+02 1.29+02 1.25+02 1.23+02 1.21+02 1.19+02 1.09+02 9 8 8.92-01 2.44+03 3.12+03 3.69+03 4.28+03 5.06+03 5.66+03 6.24+03 6.95+03 7.43+03 5.04+02 -1 -1 -1 C------------------------------------------------------------------------------- C C From a 49 term R-matrix with pseudo states (RMPS) calculation. C The close-coupling expansion included the 9 spectroscopic terms C arising from the configurations 2l, 3l, and 4l. In addition it, C included the 40 pseudo-state terms arising from the configurations C nl with n = 5 to 12 and l = 0 to 4. The spectrospic orbitals C (1s - 4f) were determined from a Thomas-Fermi Dirac-Amaldi C statistical potential. The pseudo orbitals were generated from C a set of non-orthogonal Laguerre orbitals that were then C orthogonalized to the spectroscopic orbitals and to each other. C The screening parameters for the Laguerre orbitals were adjusted C to obtain a good distribution of pseudo states above and below C the ionization limit. In STG3 of the R-Matrix calculation, C the term energies were adjusted to the experimental values. C C For all LSPI partial waves from L=0 to 11, we performed an RMPS C calculation with exchange. For the LSPI partial waves from L=12 C to 50, we performed a no-exchange RMPS calculation. These partial C waves were then topped up. The size of the continuum basis was C 45 and the size of the R-matrix "box" was 41.5 au. In the resonance C region of the calculation, we used an energy mesh spacing of C 9.0e-04 Ryd; above all thresholds of the 5l configurations, we C employed an energy-mesh spacing of 1.9e-02 Ryd up to a total C energy of 6 Ryd. The radiative rates were determined from C an LS-coupling configuration-interaction expansion that employed C all 49 terms included in the close-coupling expansion for the C RMPS calculation. C C The numbers in the last column of the above table are the theoretical C values for the reduced effective collision strengths in the infinite C temperature limit as defined in Burgess and Tully Astron. Astrophys. C 254 436 (1992). C C NAME: C Ballance and D Griffin DATE: July 22, 2003 C-------------------------------------------------------------------------------