LEADER 04417nam 22006255 450 001 9910300533703321 005 20200704052602.0 010 $a3-662-57546-9 024 7 $a10.1007/978-3-662-57546-8 035 $a(CKB)4100000005116769 035 $a(MiAaPQ)EBC5448101 035 $a(DE-He213)978-3-662-57546-8 035 $a(PPN)229498752 035 $a(EXLCZ)994100000005116769 100 $a20180706d2018 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aMillimeter Astronomy$b[electronic resource] $eSaas-Fee Advanced Course 38. Swiss Society for Astrophysics and Astronomy /$fby T. L. Wilson, Stéphane Guilloteau ; edited by Miroslava Dessauges-Zavadsky, Daniel Pfenniger 205 $a1st ed. 2018. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d2018. 215 $a1 online resource (190 pages) 225 1 $aSaas-Fee Advanced Course,$x1861-7980 ;$v38 311 $a3-662-57545-0 327 $aIntroduction 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. 330 $aThe millimeter and sub-millimeter wavebands are unique in astronomy in containing several thousands of spectral lines of molecules as well as the thermal continuum spectrum of cold dust. They are the only bands in the electromagnetic spectrum in which we can detect the molecular gas reservoir for star formation and cold dust far away in high-redshift galaxies, and nearby in low-temperature cocoons of protostars and protoplanets. This book is based on and extensively updated from the lectures given during the Saas-Fee Advanced Course 38 on millimeter astronomy. It presents both the observing techniques and the scientific perspectives of observations at millimeter wavelengths, here in particular the star and planet formation. The chapters by Thomas L. Wilson and Stéphane Guilloteau have been edited by Miroslava Dessauges-Zavadsky and Daniel Pfenniger. The book is part of the series of Saas-Fee Advanced Courses published since 1971. The targeted audience are graduate PhD and advanced undergraduate students, but the book also serves as reference for post-doctoral researchers or newcomers to the field. 410 0$aSaas-Fee Advanced Course,$x1861-7980 ;$v38 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aAstrophysics 606 $aPlanetary science 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aPlanetary Sciences$3https://scigraph.springernature.com/ontologies/product-market-codes/P22060 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 0$aAstrophysics. 615 0$aPlanetary science. 615 14$aAstronomy, Observations and Techniques. 615 24$aAstrophysics and Astroparticles. 615 24$aPlanetary Sciences. 676 $a523.01 700 $aWilson$b T. L$4aut$4http://id.loc.gov/vocabulary/relators/aut$048628 702 $aGuilloteau$b Stéphane$4aut$4http://id.loc.gov/vocabulary/relators/aut 702 $aDessauges-Zavadsky$b Miroslava$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aPfenniger$b Daniel$4edt$4http://id.loc.gov/vocabulary/relators/edt 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910300533703321 996 $aMillimeter Astronomy$92528740 997 $aUNINA