Fe II emission lines of RR Tel during an obscuration event

Details Fe II emission lines of RR Tel during an obscuration event Fe II emission lines of RR Tel during an obscuration event

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..797..577k&link_type=abstract

INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP Conference Proceedings, Volume 797, pp. 577-580 (2005).

Other

Symbiotic Stars, Novae, Variable Stars, Cataclysmic Binaries, Symbiotic Stars, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Long-Period Variables And Semiregulars

Scientific paper

A study of the behaviour of the permitted Fe II and forbidden [Fe II]
emission lines during a dust obscuration episode, suggests a larger flux
decrease for the permitted than for the forbidden lines. No other
correlation with line properties have been found. Possible
interpretations are discussed.

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