... | ... | @@ -37,7 +37,7 @@ This is mostly due to a major expansion in the physics of the H-like iso-sequenc |
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The l-levels of the H-like sequence are now fully resolved, making these atoms formally correct,
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much like the treatment of the He-sequence outlined
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in Porter et al (ApJ 622L, 73 and ApJ 644, 586).
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The predicted H~I emission line spectrum has changed as a result.
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The predicted H~I emission line spectrum has changed as a result
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Models using the large H_2 models atoms will run considerably faster, in about half the time, due to improvements in
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the memory layout.
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