<?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>Properties and nature of Be stars.
17. V360 Lac = HD 216200 is a B3e + F9IV: binary</title>
	<altname type="ADC">J/A+A/324/965</altname>
		<altname type="CDS">J/A+A/324/965</altname>
		<altname type="brief">UBV photometry of V360 Lac</altname>
	<reference>
		<source>
<journal>
	<title>Properties and nature of Be stars.
17. V360 Lac = HD 216200 is a B3e + F9IV: binary</title>
	<author>
			<initial>G</initial>
			<lastName>Hill</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>Harmanec</lastName></author>
	<author>
			<initial>K</initial>
			<lastName>Pavlovski</lastName></author>
	<author>
			<initial>H</initial>
			<lastName>Bozic</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>Hadrava</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>Koubsky</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Ziznovsky</lastName></author>
	<name>Astron. Astrophys.</name>
	<volume>324</volume>
	<pageno>965</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;A...324..965H</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Binaries_spectroscopic.html">Binaries, spectroscopic</keyword>
			<keyword xlink:href="Photometry_UBV.html">Photometry, UBV</keyword>
			<keyword xlink:href="Stars_Be.html">Stars, Be</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="binaries_eclipsing.html">binaries: eclipsing</keyword>
			<keyword xlink:href="binaries_spectroscopic.html">binaries: spectroscopic</keyword>
			<keyword xlink:href="stars_emission-line_Be.html">stars: emission-line, Be</keyword>
			<keyword xlink:href="stars_fundamental_parameters.html">stars: fundamental parameters</keyword>
			<keyword xlink:href="stars_individual_(V360_Lac).html">stars: individual (V360 Lac)</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    An analysis of an extensive collection of photometric and
    spectroscopic observations of the little studied bright Be star V360
    Lac lead to the following main conclusions:
    (1) V360 Lac is a binary system consisting of a B3e primary and a F9IV
    secondary which probably fills the Roche lobe and losses mass towards
    the primary. Radial-velocity curves of both components were obtained.
    (2) The light variations arise from superposition of variations on at
    least three time scales: phase-locked orbital brightness and colour
    changes with two minima; sinusoidal variation with a 322.24^d^ period
    and low-amplitude rapid changes with a possible period of 1.6738^d^.
    (3) A tentative solution of the B and V light curves which assumes the
    semi-detached configuration and presence of a disk around the primary,
    combined with the orbital solution, leads to preliminary basic
    physical elements of the system which are consistent with the
    radiative properties of the binary components.</para></abstract>
                        <details>
	<astroObjects>
		
			<astroObject><name>V360 Lac</name><name>14 Lac</name><name>HD 216200</name><position><ra>22 50 21.7</ra><dec>+41 57 13</dec></position></astroObject></astroObjects></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>V360 Lac: individual homogenized Johnson UBV
                                 observations from several stations</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>HJD</name>
			<definition>Heliocentric Julian date</definition>
			<units>d</units></field>
		<field>
			<name>w</name>
			<definition>weight of the data point</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>Johnson V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Bmag</name>
			<definition>Johnson B magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Umag</name>
			<definition>Johnson U magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>Johnson B-V index</definition>
			<units>mag</units></field>
		<field>
			<name>U-B</name>
			<definition>Johnson U-B index</definition>
			<units>mag</units></field>
		<field>
			<name>X</name>
			<definition>Air mass of the observation</definition>
			<units>---</units></field>
		<field>
			<name>dX</name>
			<definition>Air mass difference between var. and comp.</definition>
			<units>---</units></field>
		<field>
			<name>HD</name>
			<definition>HD number of the comparison star used</definition>
			<units>---</units></field>
		<field>
			<name>Obs</name>
			<definition>Numerical code identifying sources of data
	<footnote footnoteId="???"><para>number=1</para>
			<para>Individual observing stations are denoted by their numerical codes
           used in the Ondrejov photometric data archives as follows:
                1 ... Hvar
                3 ... Skalnate Pleso
                5 ... Lowell
                10... Kitt Peak National Observatory
                13... Mt Kobau
                33... Lick
                46... Heidelberg
                47... Akita
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>Mar</month><day>07</day></date><acknowledgement>Petr Harmanec &lt;hec@sunstel.asu.cas.cz></acknowledgement></ingest>
		</history>
	<identifier>J_A+A_324_965.xml</identifier></dataset>
