Slide 1 SiO J=5-4 in the HH211 Protostellar Jet Imaged with the SMA Naomi Hirano (ASIAA, Taiwan) (=^_^=) (=^_^=)/ Sheng-yuan Liu 1, Hsien Shang 1, PaulT.P. Ho 2, Hui-Chun…
Introduction Most of what you have heard about so far has applied to a single spectral channel with some frequency width, dn Many astronomical problems require many channels…
Outline Why spectral line (multi-channel) observing? Not only for spectral lines, but there are many advantages for continuum experiments as well Calibration specifics Bandpass,…
Star and Planet Formation Sommer term 2007 Henrik Beuther & Sebastian Wolf 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation…
Outline Why spectral line (multi-channel) observing? Not only for spectral lines, but there are many advantages for continuum experiments as well Calibration specifics Bandpass,…