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[ascl:1507.008] HLINOP: Hydrogen LINe OPacity in stellar atmospheres

HLINOP is a collection of codes for computing hydrogen line profiles and opacities in the conditions typical of stellar atmospheres. It includes HLINOP for approximate quick calculation of any line of neutral hydrogen (suitable for model atmosphere calculations), based on the Fortran code of Kurucz and Peterson found in ATLAS9. It also includes HLINPROF, for detailed, accurate calculation of lower Balmer line profiles (suitable for detailed analysis of Balmer lines) and HBOP, to implement the occupation probability formalism of Daeppen, Anderson and Milhalas (1987) and thus account for the merging of bound-bound and bound-free opacity (used often as a wrapper to HLINOP for model atmosphere calculations).

Code site:
https://github.com/barklem/hlinop
Appears in:
http://adsabs.harvard.edu/abs/2003IAUS..210P.E28B http://adsabs.harvard.edu/abs/2002A%26A...385..951B http://adsabs.harvard.edu/abs/2007A%26A...466..327B http://adsabs.harvard.edu/abs/2008A%26A...490..777L http://adsabs.harvard.edu/abs/2008A%26A...486..951G
Bibcode:
2015ascl.soft07008B

ascl:1507.008
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