<?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>Red and infrared polarimetry of highly reddened stars in the galactic plane.</title>
	<altname type="ADC">J/AJ/110/268</altname>
		<altname type="CDS">J/AJ/110/268</altname>
		<altname type="brief">Red and infrared polarimetry in galactic plane</altname>
	<reference>
		<source>
<journal>
	<title>Red and infrared polarimetry of highly reddened stars in the galactic plane.</title>
	<author>
			<initial>M</initial>
			<lastName>Creese</lastName></author>
	<author>
			<initial>T</initial>
			<initial>J</initial>
			<lastName>Jones</lastName></author>
	<author>
			<initial>H</initial>
			<initial>A</initial>
			<lastName>Kobulnicky</lastName></author>
	<name>Astron. J.</name>
	<volume>110</volume>
	<pageno>268</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995AJ....110..268C</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_infrared.html">Photometry, infrared</keyword>
			<keyword xlink:href="Polarization.html">Polarization</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We  present VRIJHK polarimetry  and JHK photometry  of highly reddened
    stars found in an  objective  prism  survey  published  by  Stephenson
    (1992AJ....103..263S). The JHK  colors of  these stars  are consistent
    with  interstellar extinction as the dominant source of the reddening.
    The distribution of  the  polarization  position  angles  in  Galactic
    coordinates is very  similar to  previous optical  polarimetry surveys
    such as Mathewson  &amp; Ford ([MNRAS,  74, 139 (1970)].  However, for the
    redder  stars  with  IR  polarimetry,  the  polarization  strength  is
    moderately lower than  expected  for  the  amount  of  extinction.  We
    postulate that the line of  sight  to  many  of  these  stars  samples
    specific regions  where  the  grain  population  has  poor  polarizing
    properties, while the remainder of the line of sight is similar to the
    paths  sampled by previous optical  surveys. The wavelength dependence
    of the polarization  from 1-2.5{mu}m  for this  sample of  stars shows
    weak  evidence for a greater departure  from the mean for interstellar
    polarization than for most published near-infrared polarimetry.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>VRIJHK polarimetry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star number from Stephenson (1992)</definition>
			<units>---</units></field>
		<field>
			<name>PolV</name>
			<definition>Polarisation in V filter</definition>
			<units>%</units></field>
		<field>
			<name>e_PolV</name>
			<definition>rms uncertainty on PV</definition>
			<units>%</units></field>
		<field>
			<name>PAV</name>
			<definition>Position angle in V filter</definition>
			<units>deg</units></field>
		<field>
			<name>PolR</name>
			<definition>Polarisation in R filter</definition>
			<units>%</units></field>
		<field>
			<name>e_PolR</name>
			<definition>rms uncertainty on PR</definition>
			<units>%</units></field>
		<field>
			<name>PAR</name>
			<definition>Position angle in R filter</definition>
			<units>deg</units></field>
		<field>
			<name>PolI</name>
			<definition>Polarisation in I filter</definition>
			<units>%</units></field>
		<field>
			<name>e_PolI</name>
			<definition>rms uncertainty on PI</definition>
			<units>%</units></field>
		<field>
			<name>PAI</name>
			<definition>Position angle in I filter</definition>
			<units>deg</units></field>
		<field>
			<name>PolJ</name>
			<definition>Polarisation in J filter</definition>
			<units>%</units></field>
		<field>
			<name>e_PolJ</name>
			<definition>rms uncertainty on PJ</definition>
			<units>%</units></field>
		<field>
			<name>PAJ</name>
			<definition>Position angle in J filter</definition>
			<units>deg</units></field>
		<field>
			<name>PolH</name>
			<definition>Polarisation in H filter</definition>
			<units>%</units></field>
		<field>
			<name>e_PolH</name>
			<definition>rms uncertainty on PH</definition>
			<units>%</units></field>
		<field>
			<name>PAH</name>
			<definition>Position angle in H filter</definition>
			<units>deg</units></field>
		<field>
			<name>PolK</name>
			<definition>Polarisation in K filter</definition>
			<units>%</units></field>
		<field>
			<name>e_PolK</name>
			<definition>rms uncertainty on PK</definition>
			<units>%</units></field>
		<field>
			<name>PAK</name>
			<definition>Position angle in K filter</definition>
			<units>deg</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>R band polarimetry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star number from Stephenson (1992)</definition>
			<units>---</units></field>
		<field>
			<name>PolR</name>
			<definition>Polarimetry in R filter</definition>
			<units>%</units></field>
		<field>
			<name>e_PolR</name>
			<definition>rms uncertainty on PR</definition>
			<units>%</units></field>
		<field>
			<name>PAR</name>
			<definition>Position angle in R filter</definition>
			<units>deg</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3">
	<title>JHK photometry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star number from Stephenson (1992)</definition>
			<units>---</units></field>
		<field>
			<name>Jmag</name>
			<definition>J magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Jmag</name>
			<definition>rms uncertainty on J magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Hmag</name>
			<definition>H magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Hmag</name>
			<definition>rms uncertainty on H magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Kmag</name>
			<definition>K magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Kmag</name>
			<definition>rms uncertainty on K magnitude</definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Apr</month><day>04</day></date><acknowledgement>Terry Jones &lt;tjj@astro.spa.umn.edu></acknowledgement></ingest>
		</history>
	<identifier>J_AJ_110_268.xml</identifier></dataset>
