Analysis of the first overtone bands of isotopologues of CO and SiO in stellar spectra

Yakiv V. Pavlenko; Sergei N. Yurchenko; Jonathan Tennyson

doi:10.1051/0004-6361/201936811

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Volume 633 (January 2020)

A&A, 633 (2020) A52

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Fig. 3

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Upper panel: dependence of the minimisation parameter computed for different spectral ranges on . Lower panel:best fit to the observed spectrum computed for = 0.0001. Profile of the ¹²C¹⁸O band is shown, in arbitrary units, by a thick cyan line. Vertical arrows mark the ¹²C¹⁸O features in the computed and observed spectrum.

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