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

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 as...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Άλλοι συγγραφείς: Niemczura, Ewa (Επιμελητής έκδοσης), Smalley, Barry (Επιμελητής έκδοσης), Pych, Wojtek (Επιμελητής έκδοσης)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: Cham : Springer International Publishing : Imprint: Springer, 2014.
Σειρά:GeoPlanet: Earth and Planetary Sciences,
Θέματα:
Διαθέσιμο Online:Full Text via HEAL-Link
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245 1 0 |a Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars  |h [electronic resource] :  |b Lectures from the School of Spectroscopic Data Analyses /  |c edited by Ewa Niemczura, Barry Smalley, Wojtek Pych. 
264 1 |a Cham :  |b Springer International Publishing :  |b Imprint: Springer,  |c 2014. 
300 |a XVI, 310 p. 128 illus., 59 illus. in color.  |b online resource. 
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490 1 |a GeoPlanet: Earth and Planetary Sciences,  |x 2190-5193 
520 |a 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. 
650 0 |a Earth sciences. 
650 0 |a Planetology. 
650 0 |a Observations, Astronomical. 
650 0 |a Astronomy  |x Observations. 
650 0 |a Space sciences. 
650 1 4 |a Earth Sciences. 
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650 2 4 |a Astronomy, Observations and Techniques. 
650 2 4 |a Extraterrestrial Physics, Space Sciences. 
700 1 |a Niemczura, Ewa.  |e editor. 
700 1 |a Smalley, Barry.  |e editor. 
700 1 |a Pych, Wojtek.  |e editor. 
710 2 |a SpringerLink (Online service) 
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776 0 8 |i Printed edition:  |z 9783319069555 
830 0 |a GeoPlanet: Earth and Planetary Sciences,  |x 2190-5193 
856 4 0 |u http://dx.doi.org/10.1007/978-3-319-06956-2  |z Full Text via HEAL-Link 
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950 |a Earth and Environmental Science (Springer-11646)