Near-Infrared Spectroscopy of TiO: Laboratory Measurements and Identification in Sunspots

Details Near-Infrared Spectroscopy of TiO: Laboratory Measurements and Identification in Sunspots Near-Infrared Spectroscopy of TiO: Laboratory Measurements and Identification in Sunspots

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apjs..107..443r&link_type=abstract

Astrophysical Journal Supplement v.107, p.443

Astronomy and Astrophysics

Astronomy

20

Methods: Laboratory, Molecular Data, Sun: Sunspots

Scientific paper

The high-resolution spectrum of the δ-system (b1π-a1Δ) of TiO, excited in a hollow cathode lamp, has been observed using a Fourier transform spectrometer. The 0-0 and 1-1 bands of this transition have also been identified in the spectrum of a sunspot umbra. The combined laboratory and solar measurements have been used to obtain improved molecular constants for the (b1π and a1Δ states of TiO.

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