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Autor:
Jeffrey D. McKaig, Shobita Satyapal, Ari Laor, Nicholas P. Abel, Sara M. Doan, Claudio Ricci, Jenna M. Cann
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 1, p 130 (2024)
Forbidden collisionally excited optical atomic transitions from high-ionization-potential (IP ≥ 54.8 eV) ions, such as Ca ^4+ , Ne ^4+ , Fe ^6+ , Fe ^10+ , Fe ^13+ , Ar ^9+ , and S ^11+ , are known as optical coronal lines (CLs). The spectral energ
Externí odkaz:
https://doaj.org/article/aff377b95a8a47b39611b5d0aab32ac2
