Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7054
Title: Quantitative astronomical spectroscopy in the post Saha equation period
Authors: Bhattacharyya, J. C
Keywords: Astronomical Spectroscopy;Saha Ionization Equation;Stellar Temperature
Issue Date: 1995
Publisher: Saha Institute of Nuclear Physics
Citation: Sinha,B and Bhattacharya, M eds, From Astronomy to Astrophysics:Proceedings of symposium on Astronomy and Astrophysics, pp. 75 - 84
Abstract: Several new questions of quantitatively estimating physical conditions on astronomical bodies had opened up after formulation of Saha Ionization Equation. The article first reviews the step by step progress in the establishment of a stellar temperature scale. The second point reviewed is the efforts by many groups for determining elemental abundances and finding the solution to the Hydrogen problem. Finally some current efforts to read the magnetic field characteristics from polarization profiles of Zeeman affected spectral lines have been described.
Description: Open Access
URI: http://hdl.handle.net/2248/7054
Appears in Collections:J.C.Bhattacharyya (1982 - 1990)
IIAP Publications

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