A search for the reported TI II 3080 multiplet emission in late-type stars

Details A search for the reported TI II 3080 multiplet emission in late-type stars A search for the reported TI II 3080 multiplet emission in late-type stars

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..781o&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Dec. 1979-Jan. 1980, p. 781-783.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Fine Structure, Late Stars, Stellar Spectra, Ultraviolet Spectra, Astronomical Spectroscopy, K Lines, Magnesium, Oao 3, Titanium

Scientific paper

Gurzadyan (1975), using a low-resolution objective-prism spectrograph, has reported the presence of both the multiplet Ti II 3080 and the doublet Mg II 2800 simultaneously either in emission or in absorption in late-type stars. Using the high-resolution spectrometers onboard Copernicus and BUSS, it is found that stars which display Mg II 2800 strongly in emission do not have a corresponding emission feature at 3080.

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