<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>CO and HI in a southern sample of interacting galaxies. I. The data</title>
	<altname type="ADC">J/A+AS/126/3</altname>
		<altname type="CDS">J/A+AS/126/3</altname>
		<altname type="brief">CO and HI in interacting galaxies</altname>
	<reference>
		<source>
<journal>
	<title>CO and HI in a southern sample of interacting galaxies. I. The data</title>
	<author>
			<initial>C</initial>
			<lastName>Horellou</lastName></author>
	<author>
			<initial>R</initial>
			<initial>S</initial>
			<lastName>Booth</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>126</volume>
	<pageno>3</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;AS..126....3H</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Carbon_monoxide.html">Carbon monoxide</keyword>
			<keyword xlink:href="Galaxies.html">Galaxies,</keyword>
			<keyword xlink:href="H_I_data.html">H I data</keyword>
			<keyword xlink:href="Radio_lines.html">Radio lines</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_evolution.html">galaxies: evolution</keyword>
			<keyword xlink:href="galaxies_interactions.html">galaxies: interactions</keyword>
			<keyword xlink:href="galaxies_ISM.html">galaxies: ISM</keyword>
			<keyword xlink:href="radio_lines_galaxies.html">radio lines: galaxies</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    Using SEST, the Parkes antenna and the Australia Telescope Compact
    Array, we have made a survey of the ^12^CO(1-0) and HI emission of an
    optically-selected sample of =~60 southern interacting and merging
    galaxies. In this paper we present the data and determine global
    masses of neutral gas (in molecular and atomic form) for the observed
    galaxies. We have detected HI in 26 systems and found that
    these galaxies have less than 15% of their gas in molecular form.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1.dat">
	<title>Galaxy Characteristics</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name</definition>
			<units>---</units></field>
		<field>
			<name>Note</name>
			<definition>Note about individual galaxies
	<footnote footnoteId="???"><para>number=1</para>
			<para>
  a : JB01   has an uncertainty in position of 30x30arcsec.
             NED gives also a radio velocity of 10079km/s
  b : JB06_2 has an uncertainty in position of 30x30arcsec
  c : JB14_2 other authors give Vhel=6321km/s
  d : JB29_1 has an uncertainty in position of 30x30arcsec
  e : JB33   has an uncertainty in position of 9x9arcsec
  f : JB40   has an uncertainty in position of 5x5arcsec
  g : JB56   HI line at Vhel=2600km/s towards JB56
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>FileName</name>
			<definition>Name of postscript figure file containing
                                        this galaxy (in this directory)</definition>
			<units>---</units></field>
		<field>
			<name>Galaxy</name>
			<definition>Galaxy name (from ESO survey)</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 1950 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension 1950 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension 1950 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 1950 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950 (minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 1950 (seconds)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Vhel</name>
			<definition>Heliocentric velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>MType</name>
			<definition>Morphological Type</definition>
			<units>---</units></field>
		<field>
			<name>logD25</name>
			<definition>Diameter at 25mag/arcsec2 (log scale)</definition>
			<units>[0.1arcmin]</units></field>
		<field>
			<name>OtherName</name>
			<definition>Other designation of the Galaxy</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3.dat">
	<title>HI and CO observational results</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>HIname</name>
			<definition>Source name</definition>
			<units>---</units></field>
		<field>
			<name>Note</name>
			<definition>Note on source
	<footnote footnoteId="???"><para>number=1</para>
			<para>the notes are
      a = pointing made toward a position between galaxies JB11_1 and JB11_2
      b = sources JB57 and JB58 observed together in HI
      d = sources not separated in HI, but are separated in CO
      n = not observed in HI
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>posFlag</name>
			<definition>Flag for uncertain (30x30") position</definition>
			<units>---</units></field>
		<field>
			<name>vHI</name>
			<definition>HI velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>DvHI</name>
			<definition>HI velocity width</definition>
			<units>km/s</units></field>
		<field>
			<name>l_SHI</name>
			<definition>Limit flag on SHI</definition>
			<units>---</units></field>
		<field>
			<name>SHI</name>
			<definition>Integrated HI flux</definition>
			<units>Jy.km/s</units></field>
		<field>
			<name>e_SHI</name>
			<definition>Mean error on HI flux</definition>
			<units>Jy.km/s</units></field>
		<field>
			<name>l_M(HI)</name>
			<definition>Limit flag on M(HI)</definition>
			<units>---</units></field>
		<field>
			<name>M(HI)</name>
			<definition>Derived HI mass</definition>
			<units>10+9solMass</units></field>
		<field>
			<name>Intrum</name>
			<definition>Instrument used (Parkes or Australian
                                        Telescope Compact Array)</definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Source name, as in table1</definition>
			<units>---</units></field>
		<field>
			<name>Note(CO)</name>
			<definition>'n' if not observed</definition>
			<units>---</units></field>
		<field>
			<name>vCO</name>
			<definition>CO velocity, observed at SEST telescope
                                        at ESO-La Silla.</definition>
			<units>km/s</units></field>
		<field>
			<name>DvCO</name>
			<definition>CO velocity width</definition>
			<units>km/s</units></field>
		<field>
			<name>l_SCO</name>
			<definition>Limit flag on SCO</definition>
			<units>---</units></field>
		<field>
			<name>SCO</name>
			<definition>Integrated antenna temperature</definition>
			<units>K.km/s</units></field>
		<field>
			<name>e_SCO</name>
			<definition>Mean error on SCO</definition>
			<units>K.km/s</units></field>
		<field>
			<name>l_M(H2)</name>
			<definition>Limit flag on M(H2) ('*' stands
                                        for tentative value)</definition>
			<units>---</units></field>
		<field>
			<name>M(H2)</name>
			<definition>Mass of H2 derived from CO data.</definition>
			<units>10+8solMass</units></field></fields></tableHead>
	
			<textFile xlink:href="fig3p1.ps" type="postscript"><name>fig3p1.ps</name><description><para>Optical images, HI and CO spectra</para></description></textFile>
			<textFile xlink:href="fig3p2.ps" type="postscript"><name>fig3p2.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p3.ps" type="postscript"><name>fig3p3.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p4.ps" type="postscript"><name>fig3p4.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p5.ps" type="postscript"><name>fig3p5.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p6.ps" type="postscript"><name>fig3p6.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p7.ps" type="postscript"><name>fig3p7.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p8.ps" type="postscript"><name>fig3p8.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p9.ps" type="postscript"><name>fig3p9.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p10.ps" type="postscript"><name>fig3p10.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p11.ps" type="postscript"><name>fig3p11.ps</name><description><para>Figure 3 continued</para></description></textFile>
			<textFile xlink:href="fig3p12.ps" type="postscript"><name>fig3p12.ps</name><description><para>Figure 3 continued</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>May</month><day>02</day></date></ingest>
		</history>
	<identifier>J_A+AS_126_3.xml</identifier></dataset>
