<?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>Further search for OH emission from IRAS sources.</title>
	<altname type="ADC">J/A+AS/124/85</altname>
		<altname type="CDS">J/A+AS/124/85</altname>
		<altname type="brief">OH emission from IRAS sources</altname>
	<reference>
		<source>
<journal>
	<title>Further search for OH emission from IRAS sources.</title>
	<author>
			<initial>V</initial>
			<initial>I</initial>
			<lastName>Slysh</lastName></author>
	<author>
			<initial>A</initial>
			<initial>M</initial>
			<lastName>Dzura</lastName></author>
	<author>
			<initial>I</initial>
			<initial>E</initial>
			<lastName>Val'tts</lastName></author>
	<author>
			<initial>E</initial>
			<lastName>Gerard</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>124</volume>
	<pageno>85</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;AS..124...85S</bibcode></journal></source>
	<related>
			<holding role="similar">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)<xlink:simple href="II/125"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Infrared_sources.html">Infrared sources</keyword>
			<keyword xlink:href="Masers.html">Masers</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="ISM_clouds.html">ISM: clouds</keyword>
			<keyword xlink:href="ISM_molecules.html">ISM: molecules</keyword>
			<keyword xlink:href="masers.html">masers</keyword>
			<keyword xlink:href="radio_lines_ISM.html">radio lines: ISM</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    Results of a continued search for OH main line emission from IRAS
    sources are reported. Towards a sample of 182 sources which consists
    of IRAS sources selected by the colour criterion for ultracompact HII
    region, and several IRAS cores, H_2_O masers and bipolar outflows, we
    detected 19 new OH masers of Class I and 5 OH/IR candidates. The
    correlation between IR and OH maser flux is confirmed. Also 51 thermal
    and 4 absorption sources were detected. The low radial velocities and
    derived OH column densities suggest that the thermal OH emission comes
    from nearby dark clouds. There is evidence that IRAS sources towards
    which thermal emission was detected are connected with these dark
    clouds.</para></abstract>
                        <details><para><observatory base="space"> IRAS</observatory></para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Masers</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>IRAS or other names</definition>
			<units>---</units></field>
		<field>
			<name>n_Name</name>
			<definition>Note
	<footnote footnoteId="???"><para>number=1</para>
			<para>a: 1665 V profile centered at -21km/s and 1665 H profile at -27km/s
              were not observed with high velocity resolution.
          b: Detection reported in the Paper I.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>GLON</name>
			<definition>Galactic longitude</definition>
			<units>deg</units></field>
		<field>
			<name>GLAT</name>
			<definition>Galactic latitude</definition>
			<units>deg</units></field>
		<field>
			<name>V(1667MHz)</name>
			<definition>Velocity (Gaussian fit for 1667MHz line)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_V(1667MHz)</name>
			<definition>rms uncertainty on V(1667MHz)</definition>
			<units>km/s</units></field>
		<field>
			<name>FWHM(1667MHz)</name>
			<definition>FWHM (Gaussian fit for 1667MHz line)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_FWHM(1667MHz)</name>
			<definition>rms uncertainty on FWHM(1667MHz)</definition>
			<units>km/s</units></field>
		<field>
			<name>l_S1667MHz</name>
			<definition>Limit flag on S1667MHz</definition>
			<units>---</units></field>
		<field>
			<name>S1667MHz</name>
			<definition>Flux (Gaussian fit for 1667MHz line)</definition>
			<units>Jy</units></field>
		<field>
			<name>e_S1667MHz</name>
			<definition>rms uncertainty on S1667MHz</definition>
			<units>Jy</units></field>
		<field>
			<name>Pol</name>
			<definition>Polarization type
	<footnote footnoteId="???"><para>number=2</para>
			<para>R: right circular polarization
          L: left circular polarization
          H: horizontal linear polarization
          V: vertical linear polarization
          T: line supposed to be thermal
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>V(1665MHz)</name>
			<definition>Velocity (Gaussian fit for 1665MHz line)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_V(1665MHz)</name>
			<definition>rms uncertainty on V(1665MHz)</definition>
			<units>km/s</units></field>
		<field>
			<name>FWHM(1665MHz)</name>
			<definition>FWHM (Gaussian fit for 1665MHz line)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_FWHM(1665MHz)</name>
			<definition>rms uncertainty on FWHM(1665MHz)</definition>
			<units>km/s</units></field>
		<field>
			<name>l_S1665MHz</name>
			<definition>Limit flag on S1665MHz</definition>
			<units>---</units></field>
		<field>
			<name>S1665MHz</name>
			<definition>Flux (Gaussian fit for 1665MHz line)</definition>
			<units>Jy</units></field>
		<field>
			<name>e_S1665MHz</name>
			<definition>rms uncertainty on S1665MHz</definition>
			<units>Jy</units></field>
		<field>
			<name>Pol2</name>
			<definition>Polarization type
	<footnote footnoteId="???"><para>number=2</para>
			<para>R: right circular polarization
          L: left circular polarization
          H: horizontal linear polarization
          V: vertical linear polarization
          T: line supposed to be thermal
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Note</name>
			<definition>c: 1665Mhz parameters are 1612MHz OH
                                              line ones (For 17269-2235 only)</definition>
			<units>---</units></field>
		<field>
			<name>OtherName</name>
			<definition>Other name</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Thermal sources</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>IRAS or other names</definition>
			<units>---</units></field>
		<field>
			<name>Lynds</name>
			<definition>Associations of an IRAS source with
                                     nebulae of Lynds</definition>
			<units>---</units></field>
		<field>
			<name>GLON</name>
			<definition>Galactic longitude</definition>
			<units>deg</units></field>
		<field>
			<name>GLAT</name>
			<definition>Galactic latitude</definition>
			<units>deg</units></field>
		<field>
			<name>l_S1667MHz</name>
			<definition>Limit flag on S1667MHz</definition>
			<units>---</units></field>
		<field>
			<name>S1667MHz</name>
			<definition>Flux at 1667MHz (result of Gaussian fits)</definition>
			<units>Jy</units></field>
		<field>
			<name>l_S1665MHz</name>
			<definition>Limit flag on S1667MHz</definition>
			<units>---</units></field>
		<field>
			<name>S1665MHz</name>
			<definition>Flux at 1665MHz (result of Gaussian fits)</definition>
			<units>Jy</units></field>
		<field>
			<name>RV</name>
			<definition>Radial velocity (result of Gaussian fits)</definition>
			<units>km/s</units></field>
		<field>
			<name>FWHM</name>
			<definition>FWHM (result of Gaussian fits)</definition>
			<units>km/s</units></field>
		<field>
			<name>N(OH)</name>
			<definition>Estimates of OH column density.</definition>
			<units>10+14cm-2</units></field>
		<field>
			<name>V(CO)</name>
			<definition>CO radial velocities</definition>
			<units>km/s</units></field>
		<field>
			<name>r_V(CO)</name>
			<definition>Reference for radial velocity
	<footnote footnoteId="???"><para>number=1</para>
			<para>1: Myers et al.  (1983ApJ...264..517)
          2: Terebey et al. (1989ApJ...340..472T)
          3: Casoli et al. (1986A&amp;A...169..281C)
          4: Heyer et al. (1987ApJ...321..370H)
          5: Wouterloot and Brand (1989, Cat. &lt;J/A+AS/80/149>)
          6: de Geus et al. (1990A&amp;A...231..137D)
          7: Benson et al. (1989)
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>IRAScloud</name>
			<definition>Name of a associated IRAS cloud or core
                                     (Wood et al. 1994, Cat. &lt;J/ApJS/95/457>)</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>Nov</month><day>12</day></date><acknowledgement>Eric Gerard &lt;Eric.Gerard@obspm.fr></acknowledgement></ingest>
		</history>
	<identifier>J_A+AS_124_85.xml</identifier></dataset>
