Studies of some diatomic molecules in the F- and early G-type dwarf stars |
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| Authors: | Markandey Singh Jai Prakash Chaturvedi |
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| Institution: | (1) Department of Physics, University of Gorakhpur, Gorakhpur, India |
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| Abstract: | A critical analysis of CH, NH, OH, C2, and CN molecules/radicals has been made in twenty-four F- and early G-type dwarfs at different effective temperature as well as in new constructed model atmosphere. Molecular indices of bandheads ofA-X system of CH, NH, OH, C2, and CN have been obtained by using the data available in the literature (thirteen-colour and eight-colour photometry).Besides, some interesting plots of the molecular indices vs  eff, molecular abundances and molecular indices vs dissociation energy, reduced equivalent widths and FCF's vs dissociation energy for respective molecules have also been enumerated. It is found that the molecular indices at bandheads ofA-X system of CH, NH, OH, C2, and CN are approximately constant (5810–6570 K). It is to be noted that the molecular indices decrease in the order OH, NH, CH, C2, and CN at a given temperature.The dissociation equilibrium of CH, NH, OH, C2, and CN is considered at 5810, 6570, and 7160 K phases in model atmosphere. At standard scale of abundance the molecular abundance and molecular index decrease in the order OH, NH, CH, C2, and CN at any given phase, however, CN abundance and index increase (eff=0.867-0.767). The amplitude of abundance and index variation decrease in the order NH, OH, CH, C2, and CN (eff=0.767-0.704).The reduced equivalent width decrease in the order OH, NH, CH, and C2 and FCF's decrease in the order CH, OH, NH, CN, and C2.The confrontation of models and observations of spectra of F- and early G-type dwarfs of parent molecules is of primary importance to investigate the physical conditions within atmospheres. Reliable excitation models are also requisite for interpreting spectroscopic observations of parent molecules and deriving molecular abundances. |
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