<?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>Studies of dense molecular cores in regions of massive star formation
II. CSJ=2-1 survey of southern H_2_O masers in the longitude range
l=260deg-310deg.</title>
	<altname type="ADC">J/A+AS/111/95</altname>
		<altname type="CDS">J/A+AS/111/95</altname>
		<altname type="brief">Studies of dense molecular cores</altname>
	<reference>
		<source>
<journal>
	<title>Studies of dense molecular cores in regions of massive star formation
II. CSJ=2-1 survey of southern H_2_O masers in the longitude range
l=260deg-310deg.</title>
	<author>
			<initial>I</initial>
			<lastName>Zinchenko</lastName></author>
	<author>
			<initial>K</initial>
			<lastName>Mattila</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Toriseva</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>111</volume>
	<pageno>95</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995A&amp;AS..111...95Z</bibcode></journal></source></reference>
	<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="stars_formation.html">stars: formation</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   We searched for the CS J=2-1 emission towards 30 southern H_2O and OH masers
   with the SEST radio telescope (29 H_2O and H_2O/OH masers and 1 OH maser).
   We detected and mapped 24 CS emitting regions associated probably with 27
   H_2O masers. The C^34^S J=2-1 and CO J=1-0 lines were also observed at the
   grid positions closest to the CS peaks.  Here we present the CS maps and the
   spectra at the peak positions along with the CO and C^34^S spectra.
   We derive the C^34^S column densities in the LTE approximation and discuss
   briefly the spatial and kinematic structure of the sources. The
   association with the IRAS point sources and small scale structure sources is
   examined. We estimate the kinematic distances to the cores and derive
   their sizes, masses and mean densities. The velocity differences between
   the masers and CS cores are analyzed. The CO and CS spectra towards
   several sources demonstrate deep absorption features. We argue that
   they can be due to extended low excitation foreground cloud(s).</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Sources</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Name of the source</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>DTheta</name>
			<definition>Uncertainty on coordinates</definition>
			<units>arcmin</units></field>
		<field>
			<name>R</name>
			<definition>Galacto-centric distance</definition>
			<units>kpc</units></field>
		<field>
			<name>Z1</name>
			<definition>Lowest value of height above the
                                  galactic plane when n_Z='/'</definition>
			<units>pc</units></field>
		<field>
			<name>n_Z</name>
			<definition>'/' indicates an interval of Z</definition>
			<units>---</units></field>
		<field>
			<name>Z</name>
			<definition>Z or higher value of Z when n_Z='/'</definition>
			<units>pc</units></field>
		<field>
			<name>Dist1</name>
			<definition>Lowest value of kinematic distances when
                                  n_Dist='/'</definition>
			<units>kpc</units></field>
		<field>
			<name>n_Dist</name>
			<definition>'/' indicates an interval of Dist</definition>
			<units>---</units></field>
		<field>
			<name>Dist</name>
			<definition>Kinematic distance or the highest value
                                  of kinematic distance when n_Dist='/'</definition>
			<units>kpc</units></field>
		<field>
			<name>Dstar1</name>
			<definition>Spectrophotometric distance of the
                                  exciting star (first detection)</definition>
			<units>kpc</units></field>
		<field>
			<name>r_Dstar1</name>
			<definition>Reference for Dstar1
	<footnote footnoteId="???"><para>number=1</para>
			<para>a) Brand J. &amp; Blitz L., 1993, A&amp;A 275, 67
          b) Avedisova V.S. &amp; Palous J., 1989,
             Bull. Astron. Inst. Czechosl. 40, 42
          c) Georgelin Y.M. &amp; Geogerlin Y.P., 1976, A&amp;A 49, 57.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Dstar2</name>
			<definition>Spectrophotometric distance of the
                                  exciting star (second detection)</definition>
			<units>kpc</units></field>
		<field>
			<name>r_Dstar2</name>
			<definition>Reference for Dstar2
	<footnote footnoteId="???"><para>number=1</para>
			<para>a) Brand J. &amp; Blitz L., 1993, A&amp;A 275, 67
          b) Avedisova V.S. &amp; Palous J., 1989,
             Bull. Astron. Inst. Czechosl. 40, 42
          c) Georgelin Y.M. &amp; Geogerlin Y.P., 1976, A&amp;A 49, 57.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Dstar3</name>
			<definition>Spectrophotometric distance of the
                                  exciting star (third detection)</definition>
			<units>kpc</units></field>
		<field>
			<name>r_Dstar3</name>
			<definition>Reference for Dstar3
	<footnote footnoteId="???"><para>number=1</para>
			<para>a) Brand J. &amp; Blitz L., 1993, A&amp;A 275, 67
          b) Avedisova V.S. &amp; Palous J., 1989,
             Bull. Astron. Inst. Czechosl. 40, 42
          c) Georgelin Y.M. &amp; Geogerlin Y.P., 1976, A&amp;A 49, 57.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>VH2Oinf</name>
			<definition>Lowest value of radial velocity of the
                                  maser when n_VH2O=','</definition>
			<units>km/s</units></field>
		<field>
			<name>n_VH2O</name>
			<definition>',' indicates an interval of values</definition>
			<units>---</units></field>
		<field>
			<name>VH2O</name>
			<definition>Radial velocity of the maser or highest value
                                  of VH2O when n_VH2O=','</definition>
			<units>km/s</units></field>
		<field>
			<name>Rem</name>
			<definition>Remarks</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Line areas and gaussian line parameters</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Source</name>
			<definition>Name of the source</definition>
			<units>---</units></field>
		<field>
			<name>Dalpha</name>
			<definition>Delta right ascension</definition>
			<units>min</units></field>
		<field>
			<name>DDE</name>
			<definition>Delta declination</definition>
			<units>arcmin</units></field>
		<field>
			<name>Int(Tmb)1</name>
			<definition>Integral of the main beam brightness
                                     temperature in dv (Line areas) (CS)</definition>
			<units>K.km/s</units></field>
		<field>
			<name>e_Int(Tmb)1</name>
			<definition>Statistical uncertainties on Line
                                     areas (CS)</definition>
			<units>0.1K.km/s</units></field>
		<field>
			<name>Tmb1</name>
			<definition>Main beam brightness temperature (CS)</definition>
			<units>K</units></field>
		<field>
			<name>e_Tmb1</name>
			<definition>Statistical uncertainties on main beam
                                     brightness temperature (CS)</definition>
			<units>0.01K</units></field>
		<field>
			<name>Vel1</name>
			<definition>LSR velocity (CS)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_Vel1</name>
			<definition>Statistical uncertainties on velocity (CS)</definition>
			<units>0.01km/s</units></field>
		<field>
			<name>DVel1</name>
			<definition>Delta velocity (CS)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_DVel1</name>
			<definition>Statistical uncertainties (CS)</definition>
			<units>0.01km/s</units></field>
		<field>
			<name>Int(Tmb)2</name>
			<definition>Integral of the main beam brightness
                                     temperature in dv (Line areas)(C^34^S)</definition>
			<units>K.km/s</units></field>
		<field>
			<name>e_Int(Tmb)2</name>
			<definition>Statistical uncertainties on Line
                                     areas (C^34^S)</definition>
			<units>0.01K.km/s</units></field>
		<field>
			<name>Tmb2</name>
			<definition>Main beam brightness temperature
                                     (C^34^S)</definition>
			<units>K</units></field>
		<field>
			<name>e_Tmb2</name>
			<definition>Statistical uncertainties on main beam
                                     brightness temperature (C^34^S)</definition>
			<units>0.01K</units></field>
		<field>
			<name>Vel2</name>
			<definition>Velocity (C^34^S)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_Vel2</name>
			<definition>Statistical uncertainties on velocity
                                     (C^34^S)</definition>
			<units>0.01km/s</units></field>
		<field>
			<name>DVel2</name>
			<definition>Delta velocity (C^34^S)</definition>
			<units>km/s</units></field>
		<field>
			<name>e_DVel2</name>
			<definition>Statistical uncertainties (C^34^S)</definition>
			<units>0.1km/s</units></field>
		<field>
			<name>Tmb3</name>
			<definition>Main beam brightness temperature (CO)</definition>
			<units>K</units></field>
		<field>
			<name>n_Tmb3</name>
			<definition>Label on the main  beam brightness
                                     temperature (CO) that indicates position
                                     (0,0)</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3">
	<title>Sources associated</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name</definition>
			<units>---</units></field>
		<field>
			<name>IRAS</name>
			<definition>IRAS name</definition>
			<units>---</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (arcmin)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (arcsec)</definition>
			<units>arcsec</units></field>
		<field>
			<name>F12</name>
			<definition>Flux at 12um for IRAS point sources</definition>
			<units>Jy</units></field>
		<field>
			<name>q_F12</name>
			<definition>Flux quality flags for F12
	<footnote footnoteId="???"><para>number=1</para>
			<para>The flux quality flags are shown following the notation in the IRAS
           point source and small scale structure catalogues
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>F25</name>
			<definition>Flux at 25um for IRAS point sources</definition>
			<units>Jy</units></field>
		<field>
			<name>q_F25</name>
			<definition>Flux quality flags for F25
	<footnote footnoteId="???"><para>number=1</para>
			<para>The flux quality flags are shown following the notation in the IRAS
           point source and small scale structure catalogues
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>F60</name>
			<definition>Flux at 60um for IRAS point sources</definition>
			<units>Jy</units></field>
		<field>
			<name>q_F60</name>
			<definition>Flux quality flags for F60
	<footnote footnoteId="???"><para>number=1</para>
			<para>The flux quality flags are shown following the notation in the IRAS
           point source and small scale structure catalogues
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>F100</name>
			<definition>Flux at 100um for IRAS point sources</definition>
			<units>Jy</units></field>
		<field>
			<name>q_F100</name>
			<definition>Flux quality flags for F100
	<footnote footnoteId="???"><para>number=1</para>
			<para>The flux quality flags are shown following the notation in the IRAS
           point source and small scale structure catalogues
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>Column densities, sizes, mean densities, masses</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Source</name>
			<definition>Source name</definition>
			<units>---</units></field>
		<field>
			<name>logNl</name>
			<definition>Column density of the core (C34S)</definition>
			<units>cm-2</units></field>
		<field>
			<name>e_logNl</name>
			<definition>Rms uncertainty on column density</definition>
			<units>0.01cm-2</units></field>
		<field>
			<name>L</name>
			<definition>Size of the core</definition>
			<units>pc</units></field>
		<field>
			<name>logn</name>
			<definition>Mean density of the core</definition>
			<units>cm-3</units></field>
		<field>
			<name>M</name>
			<definition>Mass of the core</definition>
			<units>solMass</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Mar</month><day>02</day></date></ingest>
		</history>
	<identifier>J_A+AS_111_95.xml</identifier></dataset>
