<?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>Proper Motions and UBV Photometry of Stars in the Region of Open Clusters NGC
7788, NGC 7790, Berkeley 58 and Anonymous</title>
	<altname type="ADC">5028</altname>
		<altname type="CDS">V/28</altname>
		<altname type="brief">Proper Motions, UBV Photometry, Four Open Clusters</altname>
	<reference>
		<source>
<other>
	<title>Proper Motions and UBV Photometry of Stars in the Region of Open Clusters NGC
7788, NGC 7790, Berkeley 58 and Anonymous</title>
	<author>
			<initial>V</initial>
			<initial>N</initial>
			<lastName>Frolov</lastName></author>
	<name>Pulkovo Obs., unpublished</name>
	<publisher>???</publisher>
	<city>???</city>
	
		<date>
			<year>1980</year></date>
	<bibcode>1980</bibcode></other></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_open.html">Clusters, open</keyword>
			<keyword xlink:href="Proper_motions.html">Proper motions</keyword>
			<keyword xlink:href="Photometry_UBV.html">Photometry, UBV</keyword>
			<keyword xlink:href="Regional&#10;____catalog.html">Regional
    catalog</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   Proper motions were determined for 2169 stars with limiting
   magnitude B = 16.5 mag and located within a 60 x 60 area centered at
   RA = 23 h 54.2 min, Dec = 60 deg 57 arcmin (1950.0). Three plate pairs
   with a mean epoch difference of 49 years were used. The first epoch
   plates were taken with the Tashkent normal astrograph during 1923-1925
   and the second epoch plates with the Pulkovo normal astrograph.
   The proper motions have a mean error +/-0.0030 arcsec (B &lt; 14.5 mag)
   and +/-0.0036 arcsec (B > 14.5 mag) and were measured relative to
   reference stars with 13.5 mag &lt;= B &lt;= 14.5 mag.</para><para>   Photographic UBV magnitudes were measured using Sandages photoelectric
   standards. The U, B and V magnitudes were determined for 1930, 2165 and
   1734 stars respectively, with the corresponding mean errors +/-0.03 mag,
   +/-0.06 mag and +/-0.05 mag.</para><para>   In the measured area there are three known open clusters (NGC 7788,
   NGC 7790 and Berkeley 58) and a previously unknown open cluster,
   discovered by the author, centered at RA =23 h 54.9 min, Dec = 61 deg
   21 arcmin (1950.0). The cluster members were selected on the basis of the
   proper motion (vector diagram) and photometric (V ~ B-V and U-B ~ B-V)
   criteria. Stars within areas with 4 arcmin radii centered on NGC 7788 and
   NGC 7790 and 6 arcmin radii centered on Berkeley 58 and the anonymous
   cluster were investigated for cluster membership.</para><para>   The method of reduction of the observational data and the results obtained
   have been published in Izv. Pulkovo 195, 80, 1977 and 196, 69, 1979.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="adjarea.dat">
	<title>Photometry and Proper Motions Data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>Star Number</definition>
			<units>---</units></field>
		<field>
			<name>X</name>
			<definition>X-Coordinate</definition>
			<units>mm</units></field>
		<field>
			<name>Y</name>
			<definition>Y-Coordinate</definition>
			<units>mm</units></field>
		<field>
			<name>V</name>
			<definition>V Magnitude
	<footnote>
			<para>
   The following stars are known variables
     327 - Cepheid CG Cas
     693 - Algol Type Variable
     893 - Double Cepheid CE Cas
     903 - Cepheid CF Cas</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V color index</definition>
			<units>mag</units></field>
		<field>
			<name>U-B</name>
			<definition>U-B color index</definition>
			<units>mag</units></field>
		<field>
			<name>pmX</name>
			<definition>X-annual proper motion</definition>
			<units>10-4arcmin/a</units></field>
		<field>
			<name>pmY</name>
			<definition>Y-annual proper motion</definition>
			<units>10-4arcmin/a</units></field>
		<field>
			<name>Cl_mem</name>
			<definition>Cluster Membership
	<footnote>
			<para>
   Cluster Membership Designation
     7788 = member of NGC 7788
     7790 = member of NGC 7790
       58 = member of Berkeley 58
        1 = member of anonymous cluster
        0 = no designation
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Julie Anne Watko</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1996</year><month>May</month><day>30</day></date></ingest>
		</history>
	<identifier>V_28.xml</identifier></dataset>
