<?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>Dust and CO emission in normal spirals. I. The data</title>
	<altname type="ADC">J/A+AS/118/47</altname>
		<altname type="CDS">J/A+AS/118/47</altname>
		<altname type="brief">CO observations in spirals</altname>
	<reference>
		<source>
<journal>
	<title>Dust and CO emission in normal spirals. I. The data</title>
	<author>
			<initial>R</initial>
			<lastName>Chini</lastName></author>
	<author>
			<initial>E</initial>
			<lastName>Kruegel</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Lemke</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>118</volume>
	<pageno>47</pageno>
		<date>
			<year>1996</year></date>
	<bibcode>1996A&amp;AS..118...47C</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_radio.html">Galaxies, radio</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_abundances.html">galaxies: abundances</keyword>
			<keyword xlink:href="galaxies_ISM.html">galaxies: ISM</keyword>
			<keyword xlink:href="galaxies_spiral.html">galaxies: spiral</keyword>
			<keyword xlink:href="radio_continuum_galaxies.html">radio continuum: galaxies</keyword>
			<keyword xlink:href="radio_lines_galaxies.html">radio lines: galaxies</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We present 1300{mu}m continuum observations and measurements of the
    CO (1-0) and (2-1) emission from the inner regions of 98 normal
    galaxies. The spatial resolution ranges from 11arcsec to 45arcsec.
    The sources come from a complete FIR selected sample of 138 inactive
    spirals with an optical diameter D_25_&lt;=180arcsec.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Dust emission in normal spirals</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Galaxy name</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension 1950</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension 1950</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension 1950</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 1950</definition>
			<units>arcsec</units></field>
		<field>
			<name>Dist</name>
			<definition>Distance</definition>
			<units>Mpc</units></field>
		<field>
			<name>S11</name>
			<definition>1300um flux density whithin 11" area,
                                     IRAM 30m telescope (MRT) observations</definition>
			<units>mJy</units></field>
		<field>
			<name>e_S11</name>
			<definition>rms uncertainty on S11</definition>
			<units>mJy</units></field>
		<field>
			<name>S24</name>
			<definition>1300um flux density whithin 24" area,
                                     Swedish ESO Submillimeter Telescope (SEST)
                                     observations</definition>
			<units>mJy</units></field>
		<field>
			<name>e_S24</name>
			<definition>rms uncertainty on S24</definition>
			<units>mJy</units></field>
		<field>
			<name>S70</name>
			<definition>1300um flux density whithin 70" area,
                                     SEST observations</definition>
			<units>mJy</units></field>
		<field>
			<name>e_S70</name>
			<definition>rms uncertainty on S70</definition>
			<units>mJy</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>CO emission in normal spirals</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Galaxy name</definition>
			<units>---</units></field>
		<field>
			<name>n_Name</name>
			<definition>A '*' indicates that the spectrum has been
                                   fitted by two Gaussians, and that the
                                   followed data are from the second Gaussian</definition>
			<units>---</units></field>
		<field>
			<name>Vc1</name>
			<definition>CO(1-0) MRT (24") central velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>dVc1</name>
			<definition>CO(1-0) MRT (24") line width</definition>
			<units>km/s</units></field>
		<field>
			<name>Tmb1</name>
			<definition>CO(1-0) MRT (24") temperature</definition>
			<units>mK</units></field>
		<field>
			<name>Vc2</name>
			<definition>CO(1-0) SEST (45") central velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>dVc2</name>
			<definition>CO(1-0) SEST (45") line width</definition>
			<units>km/s</units></field>
		<field>
			<name>Tmb2</name>
			<definition>CO(1-0) SEST (45") temperature</definition>
			<units>mK</units></field>
		<field>
			<name>Vc3</name>
			<definition>CO(2-1) MRT (12") central velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>dVc3</name>
			<definition>CO(2-1) MRT (12") line width</definition>
			<units>km/s</units></field>
		<field>
			<name>Tmb3</name>
			<definition>CO(2-1) MRT (12") temperature</definition>
			<units>mK</units></field>
		<field>
			<name>Vc4</name>
			<definition>CO(2-1) SEST (24") central velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>dVc4</name>
			<definition>CO(2-1) SEST (24") line width</definition>
			<units>km/s</units></field>
		<field>
			<name>Tmb4</name>
			<definition>CO(2-1) SEST (24") temperature</definition>
			<units>mK</units></field>
		<field>
			<name>I24"</name>
			<definition>I(2-1)/(1-0) integrated intensities ratio
                                     with the (1-0) lines coming from the 30m
                                     telescope and the other from SEST</definition>
			<units>---</units></field>
		<field>
			<name>ISEST</name>
			<definition>I(2-1)/(1-0) integrated intensities ratio
                                     observations refers to 45" in the (1-0)
                                     transition and 24" in (2-1)</definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="tables.tex"><name>tables.tex</name><description><para>LaTeX version of the tables</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Apr</month><day>02</day></date></ingest>
		</history>
	<identifier>J_A+AS_118_47.xml</identifier></dataset>
