/ftp/cats/A+A/591/A126



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J/A+A/591/A126      HSO line list                               (Cazzoli+, 2016)
The following files can be converted to FITS (extension .fit or fit.gz)
	list.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/591/A126
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drwxr-xr-x 36 cats archive 4096 Oct 24 2016 [Up] drwxr-xr-x 3 cats archive 208 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 467 Dec 19 2022 .message -r--r--r-- 1 cats archive 3946 Jun 24 2016 ReadMe -r--r--r-- 1 cats archive 38137 May 21 2016 hsolinel.txt -r--r--r-- 1 cats archive 32372 May 23 2016 list.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/591/A126 HSO line list (Cazzoli+, 2016) ================================================================================ Laboratory measurements and astronomical search for the HSO radical. Cazzoli G., Lattanzi V., Kirsch T., Gauss J., Tercero B., Cernicharo J., Puzzarini C. <Astron. Astrophys. 591, A126 (2016)> =2016A&A...591A.126C (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Atomic physics Keywords: submillimeter: ISM - line: identification - ISM: molecules - molecular data - methods: laboratory: molecular - radio lines: ISM Abstract: Despite the fact that many sulfur-bearing molecules, ranging from simple diatomic species up to astronomical complex molecules, have been detected in the interstellar medium, the sulfur chemistry in space is largely unknown and a depletion in the abundance of S-containing species has been observed in the cold, dense interstellar medium. The chemical form of the missing sulfur has yet to be identified. For these reasons, in view of the fact that there is a large abundance of triatomic species harbouring sulfur, oxygen, and hydrogen, we decided to investigate the HSO radical in the laboratory to try its astronomical detection. High-resolution measurements of the rotational spectrum of the HSO radical were carried out within a frequency range well up into the THz region. Subsequently, a rigorous search for HSO in the two most studied high-mass star-forming regions, Orion KL and Sagittarius (Sgr) B2, and in the cold dark cloud Barnard 1 (B1-b) was performed. Description: Complete list of measured transitions together with the spectroscopic constants in the SPFIT format.