Line identifications and intensities for the optical spectrum of RR Telescopii between 3180 and 9455 Å

Author:

Crawford F. L.,McKenna F. C.,Keenan F. P.,Aller L. H.,Feibelman W. A.,Ryan S. G.

Publisher

EDP Sciences

Subject

General Physics and Astronomy

Cited by 17 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Raman-scattered O vi Features in the Symbiotic Nova RR Telescopii;The Astrophysical Journal;2021-07-01

2. O VI RECOMBINATION LINES IN ULTRAVIOLET AND VISIBLE SPECTRA OF RR TELESCOPII;The Astrophysical Journal;2012-03-16

3. FORBIDDEN AND INTERCOMBINATION LINES OF RR TELESCOPII: WAVELENGTH MEASUREMENTS AND ENERGY LEVELS;The Astrophysical Journal Supplement Series;2011-09-30

4. Variation of Fluxes of RR Tel Emission Lines Measured in 2000 with Respect to 1996;Publications of the Astronomical Society of Japan;2009-04-25

5. CHEMICAL ABUNDANCES OF THE SYMBIOTIC NOVA AG PEGASI;Journal of The Korean Astronomical Society;2008-04-30

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