<?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>Massive stars near Eta Carinae: the stellar content of Tr 14 and Tr 16.</title>
	<altname type="ADC">J/AJ/105/980</altname>
		<altname type="CDS">J/AJ/105/980</altname>
		<altname type="brief">Massive stars near Eta Carinae: the stellar content</altname>
	<reference>
		<source>
<journal>
	<title>Massive stars near Eta Carinae: the stellar content of Tr 14 and Tr 16.</title>
	<author>
			<initial>P</initial>
			<lastName>Massey</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Johnson</lastName></author>
	<name>Astron. J.</name>
	<volume>105</volume>
	<pageno>980</pageno>
		<date>
			<year>1993</year></date>
	<bibcode>1993AJ....105..980M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_globular.html">Clusters, globular</keyword>
			<keyword xlink:href="Photometry_UBV.html">Photometry, UBV</keyword>
			<keyword xlink:href="Spectral_types.html">Spectral types</keyword></keywords>
	<descriptions>
				<description>
				<para>
    The stellar content of the region around {eta} Car is investigated
    using CCD photometry and spectroscopy.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog">
	<title>Photometry and cross-identifications
                                        (tables 1 and 2)</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star designation</definition>
			<units>---</units></field>
		<field>
			<name>X</name>
			<definition>Position (positive toward West)</definition>
			<units>pix</units></field>
		<field>
			<name>Y</name>
			<definition>Position (positive toward North)</definition>
			<units>pix</units></field>
		<field>
			<name>V</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_V</name>
			<definition>Uncertainty notes on V:
                                        "bl" indicates a blended image</definition>
			<units>---</units></field>
		<field>
			<name>U-B</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_U-B</name>
			<definition>Uncertainty notes on U-B</definition>
			<units>---</units></field>
		<field>
			<name>B-V</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_B-V</name>
			<definition>Uncertainty notes on B-V</definition>
			<units>---</units></field>
		<field>
			<name>Feinstein</name>
			<definition>Designation in clusters Tr 14 and Tr 16
                                  (A&amp;AS 12, 331, 1973 ; AJ 87, 1012, 1982)</definition>
			<units>---</units></field>
		<field>
			<name>Other</name>
			<definition>Other designation (HD or CPD)</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>The brightest and bluest stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star designation as above</definition>
			<units>---</units></field>
		<field>
			<name>X</name>
			<definition>Position (positive toward West)</definition>
			<units>pix</units></field>
		<field>
			<name>Y</name>
			<definition>Position (positive toward North)</definition>
			<units>pix</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 2000 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension 2000 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension 2000 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 2000 (sign)</definition>
			<units>-</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 2000 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 2000 (minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 2000 (seconds)</definition>
			<units>arcsec</units></field>
		<field>
			<name>V</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_V</name>
			<definition>"bl" indicates a blended image</definition>
			<units>---</units></field>
		<field>
			<name>B-V</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_B-V</name>
			<definition/>
			<units>---</units></field>
		<field>
			<name>U-B</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_U-B</name>
			<definition/>
			<units>---</units></field>
		<field>
			<name>Q</name>
			<definition>Reddening-free parameter = (U-B)-0.72*(B-V)</definition>
			<units>mag</units></field>
		<field>
			<name>Sp(New)</name>
			<definition>Spectral type from this study</definition>
			<units>---</units></field>
		<field>
			<name>Sp(W)</name>
			<definition>Spectral type from Walborn (AJ 77, 312, 1972;
                                   ApJ 179, 517, 1973; AJ 78, 1067, 1973;
                                    AJ 87, 1300, 1982)</definition>
			<units>---</units></field>
		<field>
			<name>Sp(MGL)</name>
			<definition>Spectral type from Morell, Garcia &amp; Levato,
                                    1988, PASP 100, 1431</definition>
			<units>---</units></field>
		<field>
			<name>Comment</name>
			<definition>Designations in clusters
                                  Tr 14 (A&amp;AS 12, 331, 1973) or
                                  Tr 16 (A&amp;AS 12, 331, 1973 ; AJ 87, 1012, 1982)</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table5">
	<title>New Spectral types</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star designation as above</definition>
			<units>---</units></field>
		<field>
			<name>X</name>
			<definition>Position (positive toward West)</definition>
			<units>pix</units></field>
		<field>
			<name>Y</name>
			<definition>Position (positive toward North)</definition>
			<units>pix</units></field>
		<field>
			<name>V</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_V</name>
			<definition>"bl" indicates a blended image</definition>
			<units>---</units></field>
		<field>
			<name>B-V</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_B-V</name>
			<definition>Uncertainty notes on B-V</definition>
			<units>---</units></field>
		<field>
			<name>U-B</name>
			<definition>derived from CCD photometry</definition>
			<units>mag</units></field>
		<field>
			<name>u_U-B</name>
			<definition>Uncertainty notes on U-B</definition>
			<units>---</units></field>
		<field>
			<name>Q</name>
			<definition>Reddening-free parameter = (U-B) - 0.72*(B-V)</definition>
			<units>mag</units></field>
		<field>
			<name>Sp(New)</name>
			<definition>Spectral type from this study</definition>
			<units>---</units></field>
		<field>
			<name>Comment</name>
			<definition>Designations in cluster Tr 14 or Tr 16</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table6">
	<title>Distance &amp; Reddening derived from spectroscopy</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star designation as above</definition>
			<units>---</units></field>
		<field>
			<name>E(B-V)</name>
			<definition>Color excess</definition>
			<units>mag</units></field>
		<field>
			<name>E(U-B)</name>
			<definition>Color excess</definition>
			<units>mag</units></field>
		<field>
			<name>Ratio</name>
			<definition>Ratio E(U-B)/E(B-V)</definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>Spectral type</definition>
			<units>---</units></field>
		<field>
			<name>Av</name>
			<definition>Absorption derived from spectral type</definition>
			<units>mag</units></field>
		<field>
			<name>V0</name>
			<definition>Dereddened magnitude
                                    derived from spectral type</definition>
			<units>mag</units></field>
		<field>
			<name>Mv</name>
			<definition>Absolute magnitude derived from spectral type</definition>
			<units>mag</units></field>
		<field>
			<name>m-M</name>
			<definition>Distance modulus derived from spectral type</definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>James Marcout,    Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Apr</month><day>07</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Keypunched at CDS.
        Tables 1 and 2 have been merged into a single file.</para></revision></revisions></history>
	<identifier>J_AJ_105_980.xml</identifier></dataset>
