/ftp/cats/A+A/473/177



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J/A+A/473/177       A search for pre-biotic molecules        (Wirstrom+, 2007)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	list.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/473/177
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drwxr-xr-x 14 cats archive 246 Jan 29 2012 [Up] drwxr-xr-x 3 cats archive 4096 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 467 Dec 19 2022 .message -r--r--r-- 1 cats archive 3646 Nov 25 2007 ReadMe -rw-r--r-- 1 cats archive 228 Oct 10 2017 +footg5.gif -rw-r--r-- 1 cats archive 2213 Oct 10 2017 +footg8.gif drwxr-xr-x 2 cats archive 100 Oct 10 2017 fits -rw-r--r-- 1 cats archive 178 Oct 2 2007 list.dat [txt] [txt.gz] [fits] [fits.gz] [html] -rw-r--r-- 1 cats archive 17829 Nov 26 2007 ori.tar.gz [Uncompressed]
Beginning of ReadMe : J/A+A/473/177 A search for pre-biotic molecules (Wirstrom+, 2007) ================================================================================ A search for pre-biotic molecules in hot cores. Wirstrom E.S., Bergman P., Hjalmarson A., Nummelin A. <Astron. Astrophys. 473, 177 (2007)> =2007A&A...473..177W ================================================================================ ADC_Keywords: Interstellar medium ; Radio lines ; Molecular clouds Keywords: ISM: molecules - astrobiology - molecular data Description: Low-noise, 0.8MHz resolution spectra around 90GHz towards four hot core sources: Orion KL, W51 e1/e2, S140, and W3(OH), are presented. The observations were performed using the 3mm SIS receiver at the Onsala 20m telescope. The observations were made in the beam-switching mode, the spectrum intensity is given in T_A_^*^ and high-order polynomial baselines have been subtracted. At 90GHz the Onsala 20m telescope has a beam FWHM of  42arcsec and a main-beam efficiency of  0.6. Due to changes in frequency setting during the observing period the frequency ranges are not identical for each source, but in all cases the ranges include the transitions used to determine the upper column densities of amino acetonitrile (H_2_NCH_2_CN), vinyl acetylene (C_2_H_3_CCH), oxiranecarbonitrile (c-C_3_H_3_NO), and amino-ethanol (NH_2_CH_2_CH_2_OH), presented in the paper. Note that the absorptions, seen in the S140 and the W3(OH) spectra around the strong HCN-line at 90.663GHz, are artificial. Objects: ------------------------------------------------------------------ RA (J2000) DE Designation(s) (File) ------------------------------------------------------------------ 05 35 14.5 -05 22 30 Orion KL (orionkl.dat) 19 23 44.0 +14 30 29 W51 e1/e2 (w51e1e2.dat) 22 19 19.1 +63 18 50 S140 (s140.dat) 02 27 04.4 +61 52 21 W3(OH) (w3oh.dat) ------------------------------------------------------------------