Millimeter Astronomy Saas-Fee Advanced Course 38. Swiss Society for Astrophysics and Astronomy /

The millimeter and sub-millimeter wavebands are unique in astronomy in containing several thousands of spectral lines of molecules as well as the thermal continuum spectrum of cold dust. They are the only bands in the electromagnetic spectrum in which we can detect the molecular gas reservoir for st...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
1. Verfasser: Wilson, T. L. (VerfasserIn)
Format: Elektronisch E-Book
Sprache:Englisch
Veröffentlicht: Berlin, Heidelberg : Springer Berlin Heidelberg , 2018.
Ausgabe:1st ed. 2018.
Schriftenreihe:Saas-Fee Advanced Course, 38
Schlagworte:
ISBN:9783662575468
ISSN:1861-7980 ;
Online-Zugang: Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!

MARC

LEADER 00000nam a22000005i 4500
003 SK-BrCVT
005 20220618101508.0
007 cr nn 008mamaa
008 180706s2018 gw | s |||| 0|eng d
020 |a 9783662575468 
024 7 |a 10.1007/978-3-662-57546-8  |2 doi 
035 |a CVTIDW11671 
040 |a Springer-Nature  |b eng  |c CVTISR  |e AACR2 
041 |a eng 
100 1 |a Wilson, T. L.  |4 aut 
245 1 0 |a Millimeter Astronomy  |h [electronic resource] :  |b Saas-Fee Advanced Course 38. Swiss Society for Astrophysics and Astronomy /  |c by T. L. Wilson, Stéphane Guilloteau ; edited by Miroslava Dessauges-Zavadsky, Daniel Pfenniger. 
250 |a 1st ed. 2018. 
260 1 |a Berlin, Heidelberg :  |b Springer Berlin Heidelberg ,  |c 2018. 
300 |a VII, 183 p. 54 illus., 10 illus. in color.  |b online resource. 
490 1 |a Saas-Fee Advanced Course,  |x 1861-7980 ;  |v 38 
500 |a Physics and Astronomy  
505 0 |a Introduction to Millimeter/Sub-Millimeter Astronomy (T.L. Wilson) -- 1 Introduction -- 2 Some Background -- 3 Theory of Receivers -- 4 Practical Receivers -- 5 Filled Aperture Antennas -- 6 Single Dish Observational Methods -- 7 Interferometers and Aperture Synthesis -- 8 Continuum Emission from mm/sub-mm Sources -- 9 Spectral Line Basics -- 10 Line Radiation from Atoms -- 11 Emission Nebulae, Radio Recombination Lines -- 12 Overview of Molecular Basics -- 13 Astronomical Applications -- References -- Star Formation with ALMA (S. Guilloteau) -- 1 Introduction -- 2 Dust as a Probe of Star Formation -- 3 Using Molecules -- 4 Prestellar Cores -- 5 Class 0 -- 6 Outflows -- 7 Protoplanetary Disks -- 8 High-Mass Stars -- 9 Nonstandard Observations -- 10 Conclusions: The promise of ALMA -- References. 
516 |a text file PDF 
520 |a The millimeter and sub-millimeter wavebands are unique in astronomy in containing several thousands of spectral lines of molecules as well as the thermal continuum spectrum of cold dust. They are the only bands in the electromagnetic spectrum in which we can detect the molecular gas reservoir for star formation and cold dust far away in high-redshift galaxies, and nearby in low-temperature cocoons of protostars and protoplanets. This book is based on and extensively updated from the lectures given during the Saas-Fee Advanced Course 38 on millimeter astronomy. It presents both the observing techniques and the scientific perspectives of observations at millimeter wavelengths, here in particular the star and planet formation. The chapters by Thomas L. Wilson and Stéphane Guilloteau have been edited by Miroslava Dessauges-Zavadsky and Daniel Pfenniger. The book is part of the series of Saas-Fee Advanced Courses published since 1971. The targeted audience are graduate PhD and advanced undergraduate students, but the book also serves as reference for post-doctoral researchers or newcomers to the field. 
650 0 |a Observations, Astronomical. 
650 0 |a Astronomy-Observations. 
650 0 |a Astrophysics. 
650 0 |a Planetary science. 
856 4 0 |u http://hanproxy.cvtisr.sk/han/cvti-ebook-springer-eisbn-978-3-662-57546-8  |y Vzdialený prístup pre registrovaných používateľov 
910 |b ZE08951 
919 |a 978-3-662-57546-8 
974 |a andrea.lebedova  |f Elektronické zdroje 
992 |a SUD 
999 |c 237593  |d 237593