<?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>Optical spectroscopy of radio galaxies in Abell clusters.
I. Redshifts and emission-line properties.</title>
	<altname type="ADC">J/AJ/109/14</altname>
		<altname type="CDS">J/AJ/109/14</altname>
		<altname type="brief">Optical spectroscopy of Abell clusters. I.</altname>
	<reference>
		<source>
<journal>
	<title>Optical spectroscopy of radio galaxies in Abell clusters.
I. Redshifts and emission-line properties.</title>
	<author>
			<initial>F</initial>
			<initial>N</initial>
			<lastName>Owen</lastName></author>
	<author>
			<initial>M</initial>
			<initial>J</initial>
			<lastName>Ledlow</lastName></author>
	<author>
			<initial>W</initial>
			<initial>C</initial>
			<lastName>Keel</lastName></author>
	<name>Astron. J.</name>
	<volume>109</volume>
	<pageno>14</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995AJ....109...14O</bibcode></journal></source>
	<related>
			<holding role="similar">VIII/29 : 1400-MHz Survey of 1478 Abell Galaxy Clusters (Owen+ 1982)<xlink:simple href="VIII/29"/></holding>
			<holding role="similar">J/AJ/109/853 :  VLA survey of Abell clusters. IV. (Ledlow+ 1995)<xlink:simple href="J/AJ/109/853"/></holding>
			<holding role="similar">J/AJ/110/1959 :  VLA survey of Abell clusters. V. (Ledlow+ 1995)<xlink:simple href="J/AJ/110/1959"/></holding>
			    Owen et al., Paper II.  1996AJ....111...53O</related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_galaxy.html">Clusters, galaxy</keyword>
			<keyword xlink:href="Galaxies_radio.html">Galaxies, radio</keyword>
			<keyword xlink:href="Redshifts.html">Redshifts</keyword>
			<keyword xlink:href="Spectroscopy.html">Spectroscopy</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We present results of a program of optical spectroscopy of radio
    galaxies in rich clusters. Redshifts are reported for 268 radio
    galaxies or close companions in Abell clusters and 36 objects which
    turned out to be foreground or background objects. Absolute line
    strengths are also reported for the 3727{AA} [OII] line and the
    [NII]/H{alpha} complex. We find no evidence that the radio activity in
    our sample of mostly FR I radio galaxies is associated with
    emission-line luminosities above those found in "normal" galaxies of
    the same absolute magnitude and optical type. We also find that the
    radial velocity differences between radio galaxies and the cluster
    mean seem mainly to be a function of galaxy absolute magnitude rather
    than radio properties.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Spectral parameters for radio galaxies
                                  in Abell clusters</title></tableLink>
				<tableLink xlink:href="table3">
	<title>Spectral parameters for foreground and
                                  background radio identifications</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ACO</name>
			<definition>Abell number</definition>
			<units>---</units></field>
		<field>
			<name>IAU</name>
			<definition>IAU name</definition>
			<units>---</units></field>
		<field>
			<name>m_IAU</name>
			<definition>Multiplicity index on IAU</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (1950.0)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (1950.0)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (1950.0)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (1950.0)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (1950.0)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (1950.0)</definition>
			<units>arcsec</units></field>
		<field>
			<name>z</name>
			<definition>Redshift</definition>
			<units>---</units></field>
		<field>
			<name>e_z</name>
			<definition>rms uncertainty on z</definition>
			<units>---</units></field>
		<field>
			<name>Run</name>
			<definition>Run numbers
	<footnote footnoteId="???"><para>number=1</para>
			<para>Summary of observing runs
     ----------------------------------------------------------------------
     No      Date           CCD    Grating Lines/mm {AA}/pix  Wavelength
                                                                range
     ----------------------------------------------------------------------
     1  28/01-31/01/92  Ti 800x800    09     300     2.47     3560-5525
     2  26/05-29/05/92  Ford 3x1 K   240     500     1.49     3476-7725
     3  25/09-28/09/92  Ford 3x1 K   240     500     1.49     3160-7725
     4  17/11-20/11/92  Ford 3x1 K    09     300     2.44     3425-7730
     5  24/04- 2/05/93  Ford 3x1 K    09     300     2.44     3430-7695
     </para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>l_EW1</name>
			<definition>Limit flag on EW1</definition>
			<units>---</units></field>
		<field>
			<name>EW1</name>
			<definition>H{alpha}+[NII] equivalent width</definition>
			<units>0.1pm</units></field>
		<field>
			<name>e_EW1</name>
			<definition>rms uncertainty on EW1</definition>
			<units>0.1pm</units></field>
		<field>
			<name>l_EW2</name>
			<definition>Limit flag on EW2</definition>
			<units>---</units></field>
		<field>
			<name>EW2</name>
			<definition>O[II]3727{AA} equivalent width</definition>
			<units>0.1pm</units></field>
		<field>
			<name>e_EW2</name>
			<definition>rms uncertainty on EW2</definition>
			<units>0.1pm</units></field>
		<field>
			<name>Note</name>
			<definition>Notes
	<footnote footnoteId="???"><para>number=2</para>
			<para>1 : Combined emission and absorption line redshift.
          2 : Emission line redshift.
          3 : Absorption line redshift measured manually.
          4 : Star.
          5 : Uncertain but not galaxy at cluster redshift.
          6 : Spiral
          7 : Seyfert-like spectrum
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>James Marcout, Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>Jul</month><day>29</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Prepared via OCR at CDS.</para></revision></revisions></history>
	<identifier>J_AJ_109_14.xml</identifier></dataset>
