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On the Variation of the Microturbulence Parameter with Chemical Composition

S. E. Strom

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Abstract

Stellar model atmosphere abundance analysis to correlate microturbulent velocity parameters with iron to hydrogen ratio for G dwarfs

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Stellar model atmosphere abundance analysis to correlate microturbulent velocity parameters with iron to hydrogen ratio for G dwarfs

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Available abstract

Stellar model atmosphere abundance analysis to correlate microturbulent velocity parameters with iron to hydrogen ratio for G dwarfs

Key concepts: Microturbulence, Stellar atmosphere, Astrophysics, Atmosphere (unit), Variation (astronomy), Chemical composition, Abundance (ecology), Physics

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