<?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>Planetary nebulae as standard candles. X. Tests in the Coma I region.</title>
	<altname type="ADC">J/ApJ/462/1</altname>
		<altname type="CDS">J/ApJ/462/1</altname>
		<altname type="brief">PNe in the Coma I region</altname>
	<reference>
		<source>
<journal>
	<title>Planetary nebulae as standard candles. X. Tests in the Coma I region.</title>
	<author>
			<initial>G</initial>
			<initial>H</initial>
			<lastName>Jacoby</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Ciardullo</lastName></author>
	<author>
			<initial>W</initial>
			<initial>E</initial>
			<lastName>Harris</lastName></author>
	<name>Astrophys. J.</name>
	<volume>462</volume>
	<pageno>1</pageno>
		<date>
			<year>1996</year></date>
	<bibcode>1996ApJ...462....1J</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Nebulae_planetary.html">Nebulae, planetary</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="distance_scale.html">distance scale</keyword>
			<keyword xlink:href="galaxies_clusters_individual_(Coma_I).html">galaxies: clusters: individual (Coma I)</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We present the result of an [OIII]500.7nm survey for planetary
    nebulae (PNe) in three galaxies of the Coma I group: NGC 4278 (Hubble
    type E1), NGC 4494 (E1), and NGC 4565 (edge-on Sb). Using the
    planetary nebula luminosity function (PNLF), we derived distances to
    NGC 4494 (12.8+/-0.9Mpc), NGC 4564 (10.5^+0.8^_-1.0_Mpc), and NGC 4278
    (10.2^+0.7^_-1.0_Mpc). The larger distance for NGC 4494 is significant
    beyond the 99% confidence level when the common systematic errors in
    all three distances are removed. This agrees with the results of the
    globular cluster luminosity function and surface brightness
    fluctuation methods, both of which place NGC 4565 in front of
    NGC 4494. The large separation is also consistent with the results of
    Virgocentric flow models, which predict triple-valued solutions to the
    Hubble flow in that direction.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>NGC 4278 planetary nebulae</title></tableLink>
				<tableLink xlink:href="table3">
	<title>NGC 4494 planetary nebulae</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>ID number</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (J2000)</definition>
			<units>s</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (J2000)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Rad</name>
			<definition>Isophotal radius from galaxy</definition>
			<units>arcmin</units></field>
		<field>
			<name>m5007</name>
			<definition>Lambda5007 magnitude (m5007=-2.5logF5007 - 13.74)</definition>
			<units>mag</units></field>
		<field>
			<name>Note</name>
			<definition>Note
	<footnote footnoteId="???"><para>number=1</para>
			<para>S when PNe that are part of the statistical samples
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>NGC 4565 planetary nebulae</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>ID number</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (J2000)</definition>
			<units>s</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (J2000)</definition>
			<units>arcsec</units></field>
		<field>
			<name>z</name>
			<definition>PN distance from galactic plane</definition>
			<units>arcsec</units></field>
		<field>
			<name>m5007</name>
			<definition>Lambda5007 magnitude (m5007=-2.5logF5007 - 13.74)</definition>
			<units>mag</units></field>
		<field>
			<name>Note</name>
			<definition>S when PNe that are part of the statistical
                                      samples</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table6">
	<title>Astrometric reference stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Galaxy name</definition>
			<units>---</units></field>
		<field>
			<name>ID</name>
			<definition>Star identification</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (J2000)</definition>
			<units>s</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (J2000)</definition>
			<units>arcsec</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Sep</month><day>06</day></date><acknowledgement>Robin Ciardullo &lt;rbc@astro.psu.edu></acknowledgement></ingest>
		</history>
	<identifier>J_ApJ_462_1.xml</identifier></dataset>
