N(LTE) Models with Elements H + He

These N(LTE) model atmosphere fluxes are calculated following an evolutionary track of Blöcker & Schönberner (1990, A&A 240, L11).

NLTE models are marked in red (now available!), LTE models are marked in blue (coming soon ...).

Evolutionary track

Note: The following tables are not suitable for precise spectral analyses
because approximate formulae were used in order to account for Stark line broadening.

The complete data set is available as compressed (gzip) tar archives.
use <shift>+<left mouse button> to retrieve files).

Mar 2001, solar abundances (~38 MByte)

Mar 2001, solar abundances, binned to 0.1Å intervals (5-2000Å) (~20 MByte)

Mar 2001,	solar	abundances	(~38 MByte)
Mar 2001,	solar	abundances,	binned to 0.1Å intervals (5-2000Å)	(~20 MByte)