Soft X-ray emissions of highly charged Si vii-Si xii in cool star - Procyon
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/384/2/489/3381355/mnras0384-0489.pdf
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1. High-resolution Laboratory Measurements of Coronal Lines near the Fe ix Line at 171 Å;The Astrophysical Journal;2018-02-16
2. EFFECTIVE COLLISION STRENGTHS FOR FINE-STRUCTURE TRANSITIONS IN Si VII;The Astrophysical Journal;2014-04-28
3. NEW IDENTIFICATIONS OF Fe IX, Fe X, Fe XI, Fe XII, AND Fe XIII LINES IN THE SPECTRUM OF PROCYON OBSERVED WITH THE CHANDRA X-RAY OBSERVATORY;The Astrophysical Journal Supplement Series;2014-01-09
4. SOFT X-RAY EMISSION LINES OF S VII-S XIV IN PROCYON;The Astrophysical Journal;2012-12-14
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