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Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars: Lectures from the School of Spectroscopic Data Analyses

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This book introduces the theory of stellar atmospheres. Almost everything we know about stars is by analysis of the radiation coming from their atmospheres. Several aspects of astrophysics require accurate atmospheric parameters and abundances. Spectroscopy is one of the most powerful tools at an astronomer’s disposal, allowing the determination of the fundamental parameters of stars: surface temperature, gravity, chemical composition, magnetic field, rotation and turbulence. These can be supplemented by distance measurements or pulsation parameters providing information about stellar interior and stellar evolution, otherwise unavailable.
The volume is based on lectures presented at the Wrocław's Spectroscopic School aimed at training young researchers in performing quantitative spectral analysis of low-, mid-, and high-resolution spectra of B, A, and F-type stars.

Availability
Inventory Code Barcode Call Number Location Status
1408010121EB0000136523.01 NIE dCentral LibraryAvailable
Detail Information
Series Title
-
Call Number
523.01 NIE d
Publisher
Switzerland : Springer Cham.,
Collation
xvi, 310 hlm
Language
English
ISBN/ISSN
978-3-319-06956-2
Classification
523.01
Content Type
Text
Media Type
computer
Carrier Type
online resource
Edition
1
Subject(s)
Astrofisika
Solar Physics
Specific Detail Info
-
Statement of Responsibility
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No other version available

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