24MgH+ in the solar photospheric spectrum |
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| Authors: | P D Singh |
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| Institution: | (1) Department of Astronomy, Institute of Astronomy and Geophysics, University of São Paulo, São Paulo, Brazil |
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| Abstract: | The24MgH+ (A
1 + –X
1+) molecular lines have been identified in the photospheric spectrum. The rotational excitation temperature determined from the analysis of molecular line intensities of24MgH+ is found to be of the order of 4850 K which corresponds to the photospheric temperature of the Sun. The CNDO/2 dipole moments of24MgH+ for internuclear distance range: (1.3–2.1) Å in theX
1+ state can be approximated byM(R)=4.92+1.33R. Estimations for the spontaneous emission Einstein coefficients (A
v v
) and the absorption oscillator strengths (f
v v
) for the (1, 0), (2, 0), and (2, 1) transitions in theX
1+ state of the24MgH+ ion are also made.Work partially supported by the CNPq, Brasilia under contract number 30.4076/77. |
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| Keywords: | |
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