Lyman-alpha as an Astrophysical and Cosmological Tool Saas-Fee Advanced Course 46. Swiss Society for Astrophysics and Astronomy /

• Κύριοι συγγραφείς: Dijkstra, Mark (Συγγραφέας, http://id.loc.gov/vocabulary/relators/aut), Prochaska, J. Xavier (http://id.loc.gov/vocabulary/relators/aut), Ouchi, Masami (http://id.loc.gov/vocabulary/relators/aut), Hayes, Matthew (http://id.loc.gov/vocabulary/relators/aut)
• Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
• Άλλοι συγγραφείς: Verhamme, Anne (Επιμελητής έκδοσης, http://id.loc.gov/vocabulary/relators/edt), North, Pierre (Επιμελητής έκδοσης, http://id.loc.gov/vocabulary/relators/edt), Cantalupo, Sebastiano (Επιμελητής έκδοσης, http://id.loc.gov/vocabulary/relators/edt), Atek, Hakim (Επιμελητής έκδοσης, http://id.loc.gov/vocabulary/relators/edt)
• Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
• Γλώσσα: English
• Έκδοση: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2019.
• Έκδοση: 1st ed. 2019.
• Σειρά: Saas-Fee Advanced Course, 46
• Θέματα: Observations, Astronomical.; Astronomy-Observations.; Cosmology.; Astrophysics.; Astronomy, Observations and Techniques.; Astrophysics and Astroparticles.

The hydrogen Lyman-alpha line is of utmost importance to many fields of astrophysics. This UV line being conveniently redshifted with distance to the visible and even near infrared wavelength ranges, it is observable from the ground, and provides the main observational window on the formation and ev...