<?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>Intracluster dust polarization in the Carina nebula</title>
	<altname type="ADC">J/AJ/105/258</altname>
		<altname type="CDS">J/AJ/105/258</altname>
		<altname type="brief">Intracluster dust polarization in Carina nebula</altname>
	<reference>
		<source>
<journal>
	<title>Intracluster dust polarization in the Carina nebula</title>
	<author>
			<initial>H</initial>
			<initial>G</initial>
			<lastName>Marracho</lastName></author>
	<author>
			<initial>E</initial>
			<initial>I</initial>
			<lastName>Vega</lastName></author>
	<author>
			<initial>F</initial>
			<initial>J</initial>
			<lastName>Vrba</lastName></author>
	<name>Astron. J.</name>
	<volume>105</volume>
	<pageno>258</pageno>
		<date>
			<year>1993</year></date>
	<bibcode>1993AJ....105..258M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Extinction.html">Extinction</keyword>
			<keyword xlink:href="Nebulae.html">Nebulae</keyword>
			<keyword xlink:href="Photometry_UBVRI.html">Photometry, UBVRI</keyword>
			<keyword xlink:href="Polarization.html">Polarization</keyword></keywords>
	<descriptions>
				<description>
				<para>
    This catalog presents new UBVRI polarimetric observations of 25 stars and
    BV polarimetric observations of 60 stars which are embedded in the Carina
    Nebula. Using these data and photometric data from the literature we
    have modeled and subtracted the foreground dust contribution in the
    color excess E(B-V) and the visual polarization.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>BV polarimetric observations</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Note</name>
			<definition>"*" if this is a "front-side" star
                                   (22 stars determined to be cluster members
                                   and which appear to be least affected by
                                   reddening)</definition>
			<units>---</units></field>
		<field>
			<name>HD</name>
			<definition>Henry Draper number (one star is identified as
                                   "RT Car", instead)</definition>
			<units>---</units></field>
		<field>
			<name>LS</name>
			<definition>Luminous Star (LS) number
                                   (Stephenson &amp; Sanduleak 1971).</definition>
			<units>---</units></field>
		<field>
			<name>Ident</name>
			<definition>Identification (see note 1)</definition>
			<units>---</units></field>
		<field>
			<name>P(V)</name>
			<definition>Percentage of polarization in V</definition>
			<units>%</units></field>
		<field>
			<name>e_P(V)</name>
			<definition>rms uncertainty on P(V)</definition>
			<units>%</units></field>
		<field>
			<name>Theta(V)</name>
			<definition>Equatorial position angle in V</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta(V)</name>
			<definition>rms uncertainty on Theta(V)</definition>
			<units>deg</units></field>
		<field>
			<name>P(B)</name>
			<definition>Percentage of polarization in B</definition>
			<units>%</units></field>
		<field>
			<name>e_P(B)</name>
			<definition>rms uncertainty on P(B)</definition>
			<units>%</units></field>
		<field>
			<name>Theta(B)</name>
			<definition>Equatorial position angle in B</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta(B)</name>
			<definition>rms uncertainty on Theta(B)</definition>
			<units>deg</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>UBVRI polarimetric observations</title></tableLink>
				<tableLink xlink:href="table5">
	<title>UBVRI intracluster polarization</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Note</name>
			<definition>"*" if this is a "front-side" star
                                   (22 stars determined to be cluster members
                                   and and which appear to be least affected by
                                   reddening)</definition>
			<units>---</units></field>
		<field>
			<name>HD</name>
			<definition>Henry Draper number (one star is
                                   identified as "RT Car", instead)</definition>
			<units>---</units></field>
		<field>
			<name>LS</name>
			<definition>Luminous Star (LS) number
                                   (Stephenson &amp; Sanduleak 1971).</definition>
			<units>---</units></field>
		<field>
			<name>Ident</name>
			<definition>Identification (see note 1)</definition>
			<units>---</units></field>
		<field>
			<name>P374</name>
			<definition>Percentage of polarization in
                                       lambda=0.374 um</definition>
			<units>%</units></field>
		<field>
			<name>e_P374</name>
			<definition>rms uncertainty on P374</definition>
			<units>%</units></field>
		<field>
			<name>Theta374</name>
			<definition>Equatorial position angle in
                                       lambda=0.374 um</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta374</name>
			<definition>rms uncertainty on Theta374</definition>
			<units>deg</units></field>
		<field>
			<name>P443</name>
			<definition>Percentage of polarization in lambda=443 um</definition>
			<units>%</units></field>
		<field>
			<name>e_P443</name>
			<definition>rms uncertainty on P443</definition>
			<units>%</units></field>
		<field>
			<name>Theta443</name>
			<definition>Equatorial position angle in lambda=443 um</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta443</name>
			<definition>rms uncertainty on Theta443</definition>
			<units>deg</units></field>
		<field>
			<name>P563</name>
			<definition>Percentage of polarization in lambda=0.563 um</definition>
			<units>%</units></field>
		<field>
			<name>e_P563</name>
			<definition>rms uncertainty on P563</definition>
			<units>%</units></field>
		<field>
			<name>Theta563</name>
			<definition>Equatorial position angle in lambda=0.563 um</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta563</name>
			<definition>rms uncertainty on Theta563</definition>
			<units>deg</units></field>
		<field>
			<name>P670</name>
			<definition>Percentage of polarization in lambda=0.670 um</definition>
			<units>%</units></field>
		<field>
			<name>e_P670</name>
			<definition>rms uncertainty on P670</definition>
			<units>%</units></field>
		<field>
			<name>Theta670</name>
			<definition>Equatorial position angle in lambda=0.670 um</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta670</name>
			<definition>rms uncertainty on Theta670</definition>
			<units>deg</units></field>
		<field>
			<name>P792</name>
			<definition>Percentage of polarization in lambda=0.792 um</definition>
			<units>%</units></field>
		<field>
			<name>e_P792</name>
			<definition>rms uncertainty on P792</definition>
			<units>%</units></field>
		<field>
			<name>Theta792</name>
			<definition>Equatorial position angle in lambda=0.792 um</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta792</name>
			<definition>rms uncertainty on Theta792</definition>
			<units>deg</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>Observed, foreground, and intracluster color
                                  excesses and visual polarizations</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>HD</name>
			<definition>Henry Draper number
                                   (one star is identified as "RT Car", instead)</definition>
			<units>---</units></field>
		<field>
			<name>LS</name>
			<definition>Luminous Star (LS) number
                                   (Stephenson &amp; Sanduleak 1971).</definition>
			<units>---</units></field>
		<field>
			<name>Ident</name>
			<definition>Identification (see note 1)</definition>
			<units>---</units></field>
		<field>
			<name>E(B-V)O</name>
			<definition>Observed B-V color excess</definition>
			<units>mag</units></field>
		<field>
			<name>E(B-V)F</name>
			<definition>Foreground B-V color excess</definition>
			<units>mag</units></field>
		<field>
			<name>E(B-V)I</name>
			<definition>Intracluster B-V color excess</definition>
			<units>mag</units></field>
		<field>
			<name>P(V)O</name>
			<definition>Observed polarization in V</definition>
			<units>%</units></field>
		<field>
			<name>e_P(V)O</name>
			<definition>rms uncertainty on P(V)</definition>
			<units>%</units></field>
		<field>
			<name>Theta(V)O</name>
			<definition>Observed equatorial position angle in V</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta(V)O</name>
			<definition>rms uncertainty on Theta(V)</definition>
			<units>deg</units></field>
		<field>
			<name>P(V)F</name>
			<definition>Foreground polarization in V</definition>
			<units>%</units></field>
		<field>
			<name>Theta(V)F</name>
			<definition>Foreground equatorial position angle in V</definition>
			<units>deg</units></field>
		<field>
			<name>P(V)I</name>
			<definition>Intracluster polarization in V</definition>
			<units>%</units></field>
		<field>
			<name>e_P(V)I</name>
			<definition>rms uncertainty on P(V)</definition>
			<units>%</units></field>
		<field>
			<name>Theta(V)I</name>
			<definition>Intracluster equatorial position angle in V</definition>
			<units>deg</units></field>
		<field>
			<name>e_Theta(V)I</name>
			<definition>rms uncertainty on Theta(V)</definition>
			<units>deg</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table6">
	<title>UBVRI polarization results</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>HD</name>
			<definition>Henry Draper number
                                   (one star is identified as "RT Car", instead)</definition>
			<units>---</units></field>
		<field>
			<name>LS</name>
			<definition>Luminous Star (LS) number
                                   (Stephenson &amp; Sanduleak 1971).</definition>
			<units>---</units></field>
		<field>
			<name>Ident</name>
			<definition>Identification (see note 1)</definition>
			<units>---</units></field>
		<field>
			<name>&lt;e_Theta>O</name>
			<definition>Observed dispersion of position angle
                                   normalized by the average of the position
                                   angle errors</definition>
			<units>---</units></field>
		<field>
			<name>&lt;e_Theta>I</name>
			<definition>Intracluster dispersion of position angle
                                   normalized by the average of the position
                                   angle errors</definition>
			<units>---</units></field>
		<field>
			<name>u_&lt;e_Theta>I</name>
			<definition>A colon, ':', flags two stars that have
                                   computed intracluster P(max) &lt; 0.5%, and,
                                   hence, small intracluster polarizations in
                                   relation to the external errors. The authors
                                   have chosen not to extract results from
                                   these stars.</definition>
			<units>---</units></field>
		<field>
			<name>LambdaO</name>
			<definition>Observed wavelength of maximum polarization</definition>
			<units>um</units></field>
		<field>
			<name>e_LambdaO</name>
			<definition>rms uncertainty on LambdaO</definition>
			<units>um</units></field>
		<field>
			<name>PmaxO</name>
			<definition>Observed polarization</definition>
			<units>%</units></field>
		<field>
			<name>e_PmaxO</name>
			<definition>rms uncertainty on PmaxO</definition>
			<units>%</units></field>
		<field>
			<name>Sigma1O</name>
			<definition>Observed unit weight error of
                                   least-squares fit</definition>
			<units>%</units></field>
		<field>
			<name>LambdaI</name>
			<definition>Intracluster wavelength of maximum
                                   polarization</definition>
			<units>um</units></field>
		<field>
			<name>e_LambdaI</name>
			<definition>rms uncertainty on LambdaI</definition>
			<units>um</units></field>
		<field>
			<name>PmaxI</name>
			<definition>Intracluster polarization</definition>
			<units>%</units></field>
		<field>
			<name>u_PmaxI</name>
			<definition>Uncertainty flag on PmaxI</definition>
			<units>---</units></field>
		<field>
			<name>e_PmaxI</name>
			<definition>rms uncertainty on PmaxI</definition>
			<units>%</units></field>
		<field>
			<name>Sigma1I</name>
			<definition>Intracluster unit weight error of
                                   least-squares fit</definition>
			<units>%</units></field></fields></tableHead>
	
			<textFile xlink:href="tables.tex"><name>tables.tex</name><description><para>TeX version of the tables</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Jul</month><day>06</day></date><acknowledgement>AAS CD-ROM series, Volume 1, 1993</acknowledgement></ingest>
		</history>
	<identifier>J_AJ_105_258.xml</identifier></dataset>
