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An Improved Optical Spectral Line List for RR TelescopiiThe symbiotic nova RR Telescopli has been observed with the 3.9m telescope of the Anglo-Australian Observatory (AAO), using the University College London Echelle Spectrograph in conjunction with a Tek CCD. It displays a rich emission line spectrum, ranging in excitation from N I to [Ni VIII]. We present a list of 824 measured lines, with their suggested identifications and absolute line intensities, covering a wavelength range from 3180 A to 9455 A. The absolute line intensities have been derived by comparing the high resolution data with a flux-calibrated low resolution spectrum taken with the Australian National University 2.3 m telescope. All of the lines have been successfully identified. Comparing our results with those of previous studies indicates that the RR Tel system is advancing towards higher degrees of ionization.
Document ID
19990089273
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Crawford, F. L.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
McKenna, F. C.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Keenan, F. P.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Allen, L. H.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Feibelman, W. A.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Ryan, S. G.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
August 19, 2013
Publication Date
May 24, 1999
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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