The NLTE Analyses of Carbon Emission Lines in the Atmospheres of O- and B-type Stars
Author:
Funder
NNSFC
SGSF
Young Scholars Program of Shandong University
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab41fa/pdf
Reference77 articles.
1. NLTE Line Formation for Mg i and Mg ii in the Atmospheres of B–A–F–G–K Stars
2. Carbon abundances of reference late-type stars from 1D analysis of atomic C i and molecular CH lines
3. NLTE carbon abundance determination in selected A- and B-type stars and the interpretation of C i emission lines
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1. Chemical Composition of B-type Stars from LAMOST DR5;The Astrophysical Journal;2022-10-01
2. Direct Observation of the Radial Magnetic Field Gradient in HD 58260 from Spectropolarimetry of NLTE Lines in Emission;The Astrophysical Journal;2022-01-01
3. Extended theoretical transition data in C i–iv;Monthly Notices of the Royal Astronomical Society;2021-01-28
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