<?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>Kinematical observations of pairs of galaxies.</title>
	<altname type="ADC">J/A+AS/110/19</altname>
		<altname type="CDS">J/A+AS/110/19</altname>
		<altname type="brief">Kinematical observations of pairs of galaxies</altname>
	<reference>
		<source>
<journal>
	<title>Kinematical observations of pairs of galaxies.</title>
	<author>
			<initial>E</initial>
			<lastName>Davoust</lastName></author>
	<author>
			<initial>S</initial>
			<lastName>Considere</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>110</volume>
	<pageno>19</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995A&amp;AS..110...19D</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Galaxies_spectra.html">Galaxies, spectra</keyword>
			<keyword xlink:href="Redshifts.html">Redshifts</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_distances_and_redshifts.html">galaxies: distances and redshifts</keyword>
			<keyword xlink:href="galaxies_elliptical_and_lenticular_cD.html">galaxies: elliptical and lenticular, cD</keyword>
			<keyword xlink:href="galaxies_kinematics_and_dynamics.html">galaxies: kinematics and dynamics</keyword>
			<keyword xlink:href="galaxies_spiral.html">galaxies: spiral</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We  present new radial velocities for 203  galaxies in 105 pairs and 2
    triplets. The  majority are close pairs  of early-type galaxies; there
    are  also pairs including a giant  spiral galaxy (generally M51 type),
    and  a few are wide pairs of early-type galaxies. Most velocities were
    measured from the absorption lines in the region of Mgb; emission-line
    velocities are also  given  for  22  galaxies.  The  velocity  of  one
    component only was measured  in  13  (generally  hierarchical)  pairs.
    Velocity  dispersions were measured for a  subsample of 18 close pairs
    of early-type galaxies.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Description of the observing runs</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>No</name>
			<definition>Number of the observing run</definition>
			<units>---</units></field>
		<field>
			<name>Obs</name>
			<definition>Observer
	<footnote footnoteId="???"><para>number=1</para>
			<para>JLN = Jean-Luc Nieto,
          PhP = Philippe Prugniel,
          ED = Emmanuel Davoust,
          SC = Suzanne Considere,
          OB = Olivier Bienayme
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Date</name>
			<definition>Period of observation</definition>
			<units>---</units></field>
		<field>
			<name>Disp</name>
			<definition>Dispersion</definition>
			<units>0.1nm/mm</units></field>
		<field>
			<name>sw</name>
			<definition>Slit width</definition>
			<units>arcsec</units></field>
		<field>
			<name>nS</name>
			<definition>Number of spectra</definition>
			<units>---</units></field>
		<field>
			<name>nG</name>
			<definition>number of galaxies</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Spectroscopic observations of galaxy pairs</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>n_DEd</name>
			<definition>Note on declination
	<footnote footnoteId="???"><para>number=1</para>
			<para>* = accurate coordinates (error smaller than 10arcsec) or
              accurate magnitude (error smaller than 0.3mag)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>n_Vmag</name>
			<definition>Note on V magnitude
	<footnote footnoteId="???"><para>number=1</para>
			<para>* = accurate coordinates (error smaller than 10arcsec) or
              accurate magnitude (error smaller than 0.3mag)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Sep</name>
			<definition>Separation</definition>
			<units>arcsec</units></field>
		<field>
			<name>u_Sep</name>
			<definition>Uncertainty flag on Sep</definition>
			<units>---</units></field>
		<field>
			<name>PA</name>
			<definition>Position angle</definition>
			<units>deg</units></field>
		<field>
			<name>n_PA</name>
			<definition>Orientation of the PA data</definition>
			<units>---</units></field>
		<field>
			<name>RV1(e)</name>
			<definition>e when radial velocity of emission line</definition>
			<units>---</units></field>
		<field>
			<name>RV1</name>
			<definition>Radial velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>n_RV1</name>
			<definition>Note on radial velocity
	<footnote footnoteId="???"><para>number=1</para>
			<para>* = accurate coordinates (error smaller than 10arcsec) or
              accurate magnitude (error smaller than 0.3mag)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_RV1</name>
			<definition>rms uncertainty on RV1</definition>
			<units>km/s</units></field>
		<field>
			<name>u_RV1</name>
			<definition>Uncertainty flag on RV1</definition>
			<units>---</units></field>
		<field>
			<name>nRV1</name>
			<definition>Orientation of the RV1 data</definition>
			<units>---</units></field>
		<field>
			<name>RV2(e)</name>
			<definition>e when radial velocity of emission line</definition>
			<units>---</units></field>
		<field>
			<name>RV2</name>
			<definition>Radial velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>n_RV2</name>
			<definition>Note on Radial velocity
	<footnote footnoteId="???"><para>number=1</para>
			<para>* = accurate coordinates (error smaller than 10arcsec) or
              accurate magnitude (error smaller than 0.3mag)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_RV2</name>
			<definition>rms uncertainty on RV2</definition>
			<units>km/s</units></field>
		<field>
			<name>u_RV2</name>
			<definition>Uncertainty flag on RV@</definition>
			<units>---</units></field>
		<field>
			<name>No</name>
			<definition>Observing run (see table1)
	<footnote footnoteId="???"><para>number=2</para>
			<para>The references to velocities in the literature (last column)
          are the following:
       KNF = Kollatschny et al. (1986A&amp;A...163...31K).
       M90 = Madejsky (1990).
       PDN = Prugniel et al. (1989A&amp;A...222....5P).
       PGC = Paturel et al. (1989), Cat. &lt;VII/119>
       S90 = Smith et al. (1990ApJ...356..399S).
       T85 = Tonry (1985AJ.....90.2431T).
       K followed by a number is the corresponding pair in Karachentsev
          (1987), see Cat. &lt;VII/77>
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3">
	<title>Characteristics of emission-line spectra of
                                  galaxies</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Galaxy name</definition>
			<units>---</units></field>
		<field>
			<name>EL</name>
			<definition>Identified emission lines</definition>
			<units>---</units></field>
		<field>
			<name>Class</name>
			<definition>Class
	<footnote footnoteId="???"><para>number=1</para>
			<para>1: HII, according to the line ratios of Kollatschny et al. (1986)
          2: the activity was determined from [OI]/Halpha and [OIII]/Hbeta.
          3: the emission is of circum-nuclear type, located about +/-4arcsec
              from the center; there is no emission in the very center of the
              galaxy.
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>Central velocity dispersions of galaxy pairs</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Galaxy name</definition>
			<units>---</units></field>
		<field>
			<name>n_sigma1</name>
			<definition>Orientation for sigma1 data</definition>
			<units>---</units></field>
		<field>
			<name>sigma1</name>
			<definition>Central velocity dispersion of the
                                     brighter component</definition>
			<units>km/s</units></field>
		<field>
			<name>e_sigma1</name>
			<definition>rms uncertainty on sigma1</definition>
			<units>km/s</units></field>
		<field>
			<name>n_sigma2</name>
			<definition>Orientation of the fainter component</definition>
			<units>---</units></field>
		<field>
			<name>sigma2</name>
			<definition>Central velocity dispersion of the
                                     fainter component</definition>
			<units>km/s</units></field>
		<field>
			<name>e_sigma2</name>
			<definition>rms uncertainty on sigma2</definition>
			<units>km/s</units></field>
		<field>
			<name>Ref</name>
			<definition>run/dispersion or references
	<footnote footnoteId="???"><para>number=1</para>
			<para>BN90 = Bender &amp; Nieto (1990A&amp;A...239...97B);
           B94  = Borne et al. (1994ApJ...435...79B);
           D87  = Davies et al, (1987ApJS...64..581D);
           F89  = Franx et al, (1989ApJ...344..613F);
           MK85 = Malumuth &amp; Kirshner (1985ApJ...291....8M);
           S90  = Smith et al. (1990ApJ...356..399S);
           T85  = Tonry (1985AJ.....90.2431T);
           TD81 = Tonry &amp; Davis (1981)
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>Jan</month><day>21</day></date><acknowledgement>Emmanuel Davoust &lt;davoust@srvdec.obs-mip.fr></acknowledgement></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  * 28-May-1996: First version; an error in the conversion of table2
                 resulted in missing Sep, PA and RV data
  * 21-Jan-1997: table2 corrected.</para></revision></revisions></history>
	<identifier>J_A+AS_110_19.xml</identifier></dataset>
