Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...455.1161b&link_type=abstract
Astronomy and Astrophysics, Volume 455, Issue 3, September I 2006, pp.1161-1164
Astronomy and Astrophysics
Astrophysics
2
Molecular Data, Methods: Laboratory, Techniques: Spectroscopic, Radio Lines: Ism
Scientific paper
The submillimetre-wave spectrum of the SiN radical has been investigated in the laboratory using a source-modulation microwave spectrometer equipped with a negative glow discharge cell. SiN was produced in a SiCl4/N2 discharge plasma. Twenty-one new fine and hyperfine components up to N = 17-16 were observed reaching a frequency as high as 740 GHz. The new laboratory measurements provide much improved rest frequencies in the submillimetre spectral region useful for the identification of SiN lines in hot core sources and circumstellar shells.
Bizzocchi Luca
Degli Esposti C.
Dore Luca
No associations
LandOfFree
Improved rest frequencies for the submillimetre-wave spectrum of SiN does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Improved rest frequencies for the submillimetre-wave spectrum of SiN, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Improved rest frequencies for the submillimetre-wave spectrum of SiN will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-991901