Solar Mn I 5432/5395 Åline formation explained
Open Access
- 15 April 2001
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 369 (2) , L13-L16
- https://doi.org/10.1051/0004-6361:20010223
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
This publication has 9 references indexed in Scilit:
- Spherically Symmetric Model Atmospheres for Low‐Mass Pre–Main‐Sequence Stars with Effective Temperatures between 2000 and 6800 KThe Astrophysical Journal, 2000
- TheNextGenModel Atmosphere Grid. II. Spherically Symmetric Model Atmospheres for Giant Stars with Effective Temperatures between 3000 and 6800 KThe Astrophysical Journal, 1999
- Massive Multispecies, Multilevel Non‐LTE Model Atmospheres for Novae in OutburstThe Astrophysical Journal, 1999
- Numerical solution of the expanding stellar atmosphere problemJournal of Computational and Applied Mathematics, 1999
- Solar luminosity variation. V - The photospheric lines, 1976-1985The Astrophysical Journal, 1987
- Manganese and carbon lines as temperature indicatorsSolar Physics, 1986
- Analysis of Mn I lines in the solar spectrum using accurate oscillator strengthsMonthly Notices of the Royal Astronomical Society, 1984
- Formation of the CL I line at 1351 A in the solar chromosphereThe Astrophysical Journal, 1983
- Formation of the O I resonance triplet and intercombination doublet in the solar chromosphereThe Astrophysical Journal, 1982