HII-CHI-mistry_UV: Oxygen abundance and ionizionation parameters for ultraviolet emission lines

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Ada Coda
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HII-CHI-mistry_UV: Oxygen abundance and ionizionation parameters for ultraviolet emission lines

Post by Ada Coda » Tue Jul 10, 2018 11:21 pm

HII-CHI-mistry_UV: Oxygen abundance and ionizionation parameters for ultraviolet emission lines

Abstract: HII-CHI-mistry_UV derives oxygen and carbon abundances using the ultraviolet (UV) lines emitted by the gas phase ionized by massive stars. The code first fixes C/O using ratios of appropriate emission lines and, in a second step, calculates O/H and the ionization parameter from carbon lines in the UV. An optical version of this Python code, HII-CHI-mistry (ascl:1807.007), is also available.

Credit: Pérez-Montero, Enrique; Amorín, Ricardo

Site: https://www.iaa.csic.es/~epm/HII-CHI-mistry-UV.html
https://ui.adsabs.harvard.edu/abs/2017MNRAS.467.1287P

Bibcode: 2018ascl.soft07008P

ID: ascl:1807.008
Last edited by Ada Coda on Thu Nov 19, 2020 4:25 pm, edited 1 time in total.
Reason: Updated code entry.

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