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Table · dataset · 2001

Non-LTE Ga abundance in HgMn stars

Listed in IVOA Registry (Virtual Observatory)

We present, for the first time, the Non-LTE gallium equivalent widths for the most prominent gallium transitions as identified in real spectra and in (hot) mercury-manganese star.

Description

The common feature of the departure coefficients is to decrease near the stellar surface, the collision rates are dominant in many cases and the Non-LTE equivalent widths are generally smaller. In particular, the abundance difference as derived from UV and visual lines is reduced.

The photoionization cross sections were computed by means of standard R-matrix formalism.

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