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We present an overview of a few spectroscopic diagnostics of massive stars. We explore the following wavelength ranges: UV (1000 to 2000 A), optical (4000--7000 A) and near-infrared (mainly H and K ba...
The coming years will see routine use of solar data of unprecedented spatial and spectral resolution, time cadence, and completeness in the wavelength domain. To capitalize on the soon to be availabl...
Context. Mass loss of ∼ 0.1-0.3 M⊙ from Population II red giant stars (RGB) is a requirement of stellar evolution theory in order to account for several observational evidences in globular clust...
An assessment on the capabilities of modern spectropolarimeters and magnetographs is in order since most of our astrophysical results rely upon the accuracy of the instrumentation and on the sensitivi...
Magnetic field in the solar lower atmosphere can be measured by the use of the Zeeman and Hanle effects. In contrast, the coronal magnetic field well above the solar surface, which directly controls v...
Temperature diagnostics of the Broad Line Region in Active Galactic Nuclei。
Diagnostics of the Ionized ISM:The Importance of Density Fluctuations
Spectroscopic diagnostics of precessing discs:the Stream-disc impact in xtej1118+480 (= kV uma) in outburst
X-ray plasma diagnostics for totally and partially photoionized plasmas such as warm absorbers in agn

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