Publication Date:
2019-08-17
Description:
As part of a project to complete a comprehensive catalogue of astrophysically relevant emission lines in support of new-generation X-ray observatories using the Lawrence Livermore electron beam ion traps EBIT-I and EDIT-II, emission lines of argon and sulfur in the soft X-ray and extreme ultraviolet region were studied. Observations of Ar IX through Ar XVI and S VII through S XIV between 20 and 75 Angstrom are presented to illustrate our work.
Keywords:
Astronomy
Type:
Proceedings of the NASA Laboratory Astrophysics Workshop; 67-69; NASA/CP-2002-211863
Format:
application/pdf