========================================================================== J/A+A/540/A96 Molecular gas in Hickson Compact Groups (Martinez-Badenes+, 2012) The following files can be converted to FITS (extension .fit or fit.gz) table1.dat table2.dat table3.dat table5.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/540/A96 ==========================================================================
drwxr-xr-x 23 cats archive 4096 Oct 26 2012 [Up] drwxr-xr-x 3 cats archive 4096 May 12 09:59 [TAR file] -rw-r--r-- 1 cats archive 499 Jul 1 2012 .message -r--r--r-- 1 cats archive 11855 Jul 1 2012 ReadMe -rw-r--r-- 1 cats archive 319 Jul 1 2012 +footg5.gif -rw-r--r-- 1 cats archive 2486 Jul 1 2012 +footg8.gif -r--r--r-- 1 cats archive 4755 Mar 12 2012 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 6321 Mar 12 2012 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4343 Mar 12 2012 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2349 Mar 12 2012 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/540/A96 Molecular gas in Hickson Compact Groups (Martinez-Badenes+, 2012) ================================================================================ Molecular gas content and SFR in Hickson Compact Groups: enhanced or deficient? Martinez-Badenes V. Lisenfeld U., Espada D., Verdes-Montenegro L., Garcia-Burillo S., Leon S., Sulentic J., Min Y.S. <Astron. Astrophys. 540, A96 (2012)> =2012A&A...540A..96M ================================================================================ ADC_Keywords: Clusters, galaxy ; Carbon monoxide ; H I data ; Infrared sources Keywords: ISM: molecules - galaxies: evolution - galaxies: ISM - galaxies: interactions - galaxies: star formation - galaxies: groups: general Abstract: We study the effect of the extreme environment in Hickson Compact Groups (HCGs) on the molecular gas mass, M_H2_, and the star formation rate (SFR) of galaxies as a function of atomic hydrogen (HI) content and evolutionary phase of the group. We selected a redshift-limited (D<100Mpc) sample of 88 galaxies in 20 HCGs with available atomic hydrogen (HI) VLA maps, covering a wide range of HI deficiencies and evolutionary phases of the groups containing at least one spiral galaxy. We observed the CO(1-0) and CO(2-1) lines with the IRAM 30m telescope for 47 galaxies. Together with literature data, our sample contains CO(1-0) spectra for 86 galaxies. We derived the far-infrared (FIR) luminosity L_FIR_ from IRAS data and used it as a tracer of the star formation rate (SFR). We calculated the HI mass, M_HI_ L_FIR_ and M_H2_ deficiencies, based on the values expected from L_B_ and L_K_ in isolated galaxies from the AMIGA sample. We limited our statistical analysis to spiral galaxies, since the large number of upper limits did not allow drawing strong conclusions about M_H2_ and L_FIR_ in early-type galaxies.
© UDS/CNRS