<?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>uvby-beta photometry of Orion population stars and related objects associated
with six galactic star-forming regions</title>
	<altname type="ADC">J/A+AS/104/557</altname>
		<altname type="CDS">J/A+AS/104/557</altname>
		<altname type="brief">uvby-beta photometry in star-forming regions</altname>
	<reference>
		<source>
<journal>
	<title>uvby-beta photometry of Orion population stars and related objects associated
with six galactic star-forming regions</title>
	<author>
			<initial>L</initial>
			<lastName>Terranegra</lastName></author>
	<author>
			<initial>C</initial>
			<lastName>Chavarria-K</lastName></author>
	<author>
			<initial>S</initial>
			<lastName>Diaz</lastName></author>
	<author>
			<initial>D</initial>
			<lastName>Gonzalez-Patino</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>104</volume>
	<pageno>557</pageno>
		<date>
			<year>1994</year></date>
	<bibcode>1994A&amp;AS..104..557T</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="dust_extinction.html">dust, extinction</keyword>
			<keyword xlink:href="stars_emission-line_Be.html">stars: emission-line, Be</keyword>
			<keyword xlink:href="stars_pre-main_sequence.html">stars: pre-main sequence</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   Homogeneous uvby{beta} photometry of 150 stars associated with the star
   forming regions Taurus-Auriga, Orion, Canis Mayoris, Ophiuchus, Serpens
   and Cygnus, is presented here. We also present uvby{beta} photometry of
   10 Herbig Ae/Be stars not belonging to the specific regions studied here.
   Using the (V,b-y), ({beta},[m1]), ([c1],[m1]) and ([u-b], T_eff_) diagrams
   we study the photometric properties of the sample. The effects of duplicity,
   stellar rotation, and interstellar extinction on the location in the
   magnitude-color and color-color diagrams of our program stars are briefly
   investigated. We derive reliable photometric spectral types and discuss
   membership to the regions and to the Orion population, as well as
   peculiarities of the individual stars. We also find new B stars associated
   with the CMa R1 star forming region and new intermediate-low mass PMS
   members associated with the BD+404124/BD+413731 region. The FU-Orionis
   stars Z CMa, V1515 Cyg and V1057 Cyg have a peculiar position in the
   reddening free ({beta},[m1]) diagram. With diagrams such as (V-M _v_-5 log
   r+5) vs. E(b-y), E(c1) vs. E(b-y), E(m1) vs. E(b-y) and E(u-b) vs. E(b-y)
   we investigate the IS extinction law towards the star-forming regions. We
   find that the total to selective extinction ratio to these regions is
   steeper than normal with R_y_=5.4 (R_v_=4.0) and the coefficients
   E(c1)/E(b-y) and E(m1)/E(b-y) used to define the reddening free indices
   [c1] and [m1] should be numerically smaller than the generally adopted
   values.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3a">
	<title>Mean uvby-beta photometry of 150 Orion
                                  population stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Group</name>
			<definition>Group number
	<footnote footnoteId="???"><para>number=1</para>
			<para>See note (1) for table3b
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>Photometric spectral type</definition>
			<units>---</units></field>
		<field>
			<name>Note</name>
			<definition>Note</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Vmag</name>
			<definition>rms uncertainty on V</definition>
			<units>mag</units></field>
		<field>
			<name>(b-y)</name>
			<definition>(b-y) index</definition>
			<units>mag</units></field>
		<field>
			<name>e_(b-y)</name>
			<definition>rms uncertainty on (b-y)</definition>
			<units>mag</units></field>
		<field>
			<name>c1</name>
			<definition>c1 index</definition>
			<units>mag</units></field>
		<field>
			<name>e_c1</name>
			<definition>rms uncertainty on c1</definition>
			<units>mag</units></field>
		<field>
			<name>m1</name>
			<definition>m1 index</definition>
			<units>mag</units></field>
		<field>
			<name>e_m1</name>
			<definition>rms uncertainty on m1</definition>
			<units>mag</units></field>
		<field>
			<name>beta</name>
			<definition>beta index</definition>
			<units>mag</units></field>
		<field>
			<name>n_beta</name>
			<definition>When *, the stars was not observed in
                                           Beta index</definition>
			<units>---</units></field>
		<field>
			<name>e_beta</name>
			<definition>rms uncertainty on Beta</definition>
			<units>mag</units></field>
		<field>
			<name>Nobs</name>
			<definition>Number of observations</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3b">
	<title>Complete uvby-beta photometry of 150 Orion
                                  population stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Group</name>
			<definition>Group number
	<footnote footnoteId="???"><para>number=1</para>
			<para>
       1 = Taurus-Auriga
       2 = Orion
       3 = CMa R1
       4 = NGC 6611
       5 = Ophiuchus
       6 = BD+40 4124 and BD+41 3731 groups
       7 = NGC 7000/IC 5070
       8 = Miscellaneous stars
       9 = Miscellaneous Herbig Ae/Be stars
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension 1950</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension 1950</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension 1950</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 1950</definition>
			<units>arcsec</units></field>
		<field>
			<name>Sp</name>
			<definition>Photometric spectral type</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>(b-y)</name>
			<definition>(b-y) index</definition>
			<units>mag</units></field>
		<field>
			<name>c1</name>
			<definition>c1 index</definition>
			<units>mag</units></field>
		<field>
			<name>m1</name>
			<definition>m1 index</definition>
			<units>mag</units></field>
		<field>
			<name>beta</name>
			<definition>beta index</definition>
			<units>mag</units></field>
		<field>
			<name>JDhel</name>
			<definition>Heliocentric Julian day</definition>
			<units>d</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer, Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Jul</month><day>07</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  * 18-Feb-1994: first prepared
  * 07-Jul-1995: replaced 2440000-offset dates by complete ones</para></revision></revisions></history>
	<identifier>J_A+AS_104_557.xml</identifier></dataset>
