<?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>New periods of variable stars in Cygnus based on a quarter of century of
photographic observations.</title>
	<altname type="ADC">J/A+AS/135/29</altname>
		<altname type="CDS">J/A+AS/135/29</altname>
		<altname type="brief">New periods of variable stars in Cygnus</altname>
	<reference>
		<source>
<journal>
	<title>New periods of variable stars in Cygnus based on a quarter of century of
photographic observations.</title>
	<author>
			<initial>L</initial>
			<lastName>Hric</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Galis</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>135</volume>
	<pageno>29</pageno>
		<date>
			<year>1999</year></date>
	<bibcode>1999A&amp;AS..135...29H</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Magnitudes.html">Magnitudes</keyword>
			<keyword xlink:href="Stars_variable.html">Stars, variable</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="stars_variables_general.html">stars: variables: general</keyword>
			<keyword xlink:href="techniques_photometric.html">techniques: photometric</keyword></keywords>
	<descriptions>
				<description>
				<para>
    The Table2 summarizes the photographic magnitudes obtained over 24
    years at the Skalnate Pleso (1979-1993) and Asiago (1969-1988)
    observatories for 17 variable stars of different types: Miras (7),
    Semi-regular (4), Cepheids (3), RR Lyr (2), Eclipsing binary (1).
    The cross-reference between star No., designation according to Margoni
    and Stagni (1984A&amp;AS...56...87M) and catalogue one (provided it has
    already been adopted for a given star) according to the GCVS (See Cat.
    &lt;II/214>) and IBVS (Kholopov al., 1987, See Cat. &lt;II/195>) is given in
    Table3 as well as the equatorial coordinates for the epoch 1950.0 for
    each star, which is compatible with the GCVS. In this table are shown
    the basic characteristics of the observational material for each star:
    the number of data points and interval of magnitudes obtained at the
    Asiago Observatory (A) and Skalnate Pleso Observatory (SP) respectively.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2.dat">
	<title>Photographic magnitudes for 17 variables</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>JD</name>
			<definition>Date</definition>
			<units>d</units></field>
		<field>
			<name>No1</name>
			<definition>Magnitude for star No.1</definition>
			<units>mag</units></field>
		<field>
			<name>No2</name>
			<definition>Magnitude for star No.2</definition>
			<units>mag</units></field>
		<field>
			<name>No3</name>
			<definition>Magnitude for star No.3</definition>
			<units>mag</units></field>
		<field>
			<name>No4</name>
			<definition>Magnitude for star No.4</definition>
			<units>mag</units></field>
		<field>
			<name>No5</name>
			<definition>Magnitude for star No.5</definition>
			<units>mag</units></field>
		<field>
			<name>No6</name>
			<definition>Magnitude for star No.6</definition>
			<units>mag</units></field>
		<field>
			<name>No7</name>
			<definition>Magnitude for star No.7</definition>
			<units>mag</units></field>
		<field>
			<name>No8</name>
			<definition>Magnitude for star No.8</definition>
			<units>mag</units></field>
		<field>
			<name>No9</name>
			<definition>Magnitude for star No.9</definition>
			<units>mag</units></field>
		<field>
			<name>No10</name>
			<definition>Magnitude for star No.10</definition>
			<units>mag</units></field>
		<field>
			<name>No11</name>
			<definition>Magnitude for star No.11</definition>
			<units>mag</units></field>
		<field>
			<name>No12</name>
			<definition>Magnitude for star No.12</definition>
			<units>mag</units></field>
		<field>
			<name>No13</name>
			<definition>Magnitude for star No.13</definition>
			<units>mag</units></field>
		<field>
			<name>No14</name>
			<definition>Magnitude for star No.14</definition>
			<units>mag</units></field>
		<field>
			<name>No15</name>
			<definition>Magnitude for star No.15</definition>
			<units>mag</units></field>
		<field>
			<name>No16</name>
			<definition>Magnitude for star No.16</definition>
			<units>mag</units></field>
		<field>
			<name>No17</name>
			<definition>Magnitude for star No.17</definition>
			<units>mag</units></field>
		<field>
			<name>Obs</name>
			<definition>Observatory; See Note
	<footnote footnoteId="???"><para>number=1</para>
			<para>A : Asiago Observatory
          SP: Skalnate Pleso Observatory
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3.dat">
	<title>The basic characteristics of investigated stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>No</name>
			<definition>Star No.</definition>
			<units>---</units></field>
		<field>
			<name>[MS84]</name>
			<definition>Margoni and Stagni (1984A&amp;AS...56...87M)
                                     designation</definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>GCVS/IBVS designation</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension 1950 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension 1950 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension 1950 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 1950 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950 (arcminutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>NobsA</name>
			<definition>Number of observations (Asiago Obs.)</definition>
			<units>---</units></field>
		<field>
			<name>maxA</name>
			<definition>Maximal brightness (Asiago Obs.)</definition>
			<units>mag</units></field>
		<field>
			<name>minA</name>
			<definition>Minimal brightness (Asiago Obs.)</definition>
			<units>mag</units></field>
		<field>
			<name>NobsSP</name>
			<definition>Number of observations (Skalnate Pleso Obs.)</definition>
			<units>---</units></field>
		<field>
			<name>maxSP</name>
			<definition>Maximal brightness (Skalnate Pleso Obs.)</definition>
			<units>mag</units></field>
		<field>
			<name>minSP</name>
			<definition>Minimal brightness (Skalnate Pleso Obs.)</definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1998</year><month>Dec</month><day>03</day></date><acknowledgement>Ladislav Hric &lt;hric@ta3.sk></acknowledgement></ingest>
		</history>
	<identifier>J_A+AS_135_29.xml</identifier></dataset>
