<?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>Catalogue of nearest stars until 10pc</title>
	<altname type="ADC">5101</altname>
		<altname type="CDS">V/101</altname>
		<altname type="brief">Nearest stars until 10pc</altname>
	<reference>
		<source>
<journal>
	<title>Catalogue of nearest stars until 10pc</title>
	<author>
			<initial>V</initial>
			<initial>A</initial>
			<lastName>Zakhozhaj</lastName></author>
	<name>Vestnik Khar'kovskogo Universiteta</name>
	<volume>190</volume>
	<pageno>52</pageno>
		<date>
			<year>1979</year></date>
	<bibcode>1979VKha..190...52Z</bibcode></journal></source>
	<related>
			<holding role="similar">V/70 : Nearby Stars, Preliminary 3rd Version (Gliese+ 1991)<xlink:simple href="V/70"/></holding>
			<holding role="similar">J/other/KFNT/12.20 :  Nearby stars metallicities (Zakhozhaj+ 1996)<xlink:simple href="J/other/KFNT/12.20"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Stars_nearby.html">Stars, nearby</keyword>
			<keyword xlink:href="Stars_masses.html">Stars, masses</keyword>
			<keyword xlink:href="Stars_diameters.html">Stars, diameters</keyword>
			<keyword xlink:href="Proper_motions.html">Proper motions</keyword>
			<keyword xlink:href="Parallaxes_spectroscopic.html">Parallaxes, spectroscopic</keyword>
			<keyword xlink:href="Parallaxes_trigonometric.html">Parallaxes, trigonometric</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="Stars_nearby_masses_radii.html">Stars, nearby, masses, radii</keyword>
			<keyword xlink:href="astrometry.html">astrometry</keyword>
			<keyword xlink:href="Spectral_types.html">Spectral types</keyword>
			<keyword xlink:href="Magnitudes_absolute.html">Magnitudes, absolute</keyword></keywords>
	<descriptions>
				<description>
				<para>
    The given catalogue is a revised version of the catalogue (Zakhozhaj,
    1987). The previous numeration is preserved, and the stars, with
    trigonometric, photometric and spectral parallaxes >0.100" are
    presented. The catalogue contains data on new components of multiple
    visual systems, on the components of spectral-binary systems, on
    invisible components with masses >0.08 solar mass. New data are
    obtained in 90s and contained in the articles [2-6]. The catalogue
    contains the main characteristics of stars such as the positions,
    proper motions, radial velocities, parallaxes, photometrical data and
    also new data of masses and radii of stars. The completeness of the
    catalogue is about 70%.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>Catalogue of stars within ten parsecs of the Sun</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Zkh</name>
			<definition>Running number (Zakhozhaj's catalog)</definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Star identifier</definition>
			<units>---</units></field>
		<field>
			<name>m_Name</name>
			<definition>Component of multiple star</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>Rem</name>
			<definition>Remark
	<footnote footnoteId="???"><para>number=1</para>
			<para>Coordinates of multiple system components are calculated on the basis
            of the angular separation and position of observation epoch.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>pmRA</name>
			<definition>Proper motion pmRA.cos(DE)</definition>
			<units>s/yr</units></field>
		<field>
			<name>n_pmRA</name>
			<definition>Notes
	<footnote footnoteId="???"><para>number=2</para>
			<para>*: pmRA and pmDE for multiple system components are calculated by
               the common proper motion and the position angle.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>pmDE</name>
			<definition>Proper motion pmDE</definition>
			<units>arcsec/a</units></field>
		<field>
			<name>n_pmDE</name>
			<definition>Notes
	<footnote footnoteId="???"><para>number=2</para>
			<para>*: pmRA and pmDE for multiple system components are calculated by
               the common proper motion and the position angle.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RV</name>
			<definition>Heliocentric Radial velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>Gliese</name>
			<definition>Gliese (Cat. &lt;V/70>) identifier</definition>
			<units>---</units></field>
		<field>
			<name>m_Gliese</name>
			<definition>Gliese star component</definition>
			<units>---</units></field>
		<field>
			<name>Plx</name>
			<definition>Stellar parallax</definition>
			<units>mas</units></field>
		<field>
			<name>n_Plx</name>
			<definition>Index to parallax
	<footnote footnoteId="???"><para>number=3</para>
			<para>t: trigonometric parallax
          p: photometric parallax
          s: spectral parallax
          r: average value of t, p and s parallaxes
          a: average value of p and s parallaxes
          o: photometric or spectral parallax</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>u_Plx</name>
			<definition>Notes to Plx
	<footnote footnoteId="???"><para>number=4</para>
			<para>*: The values of parallaxes with error of 10% and more.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>l_Vmag</name>
			<definition>Limit flag on Vmag</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>n_Vmag</name>
			<definition>Note on magnitude
	<footnote footnoteId="???"><para>number=5</para>
			<para>v: variable star
          S: summarized magnitude of components,
          n: author' estimation of Vmag and Mv are made for visible component
               or for component for which it is possible to estimate component
               spectrum.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>l_Mv</name>
			<definition>Limit flag on Mv</definition>
			<units>---</units></field>
		<field>
			<name>Mv</name>
			<definition>Absolute magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>n_Mv</name>
			<definition>Note on magnitude
	<footnote footnoteId="???"><para>number=5</para>
			<para>v: variable star
          S: summarized magnitude of components,
          n: author' estimation of Vmag and Mv are made for visible component
               or for component for which it is possible to estimate component
               spectrum.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>Spectral classification</definition>
			<units>---</units></field>
		<field>
			<name>n_Sp</name>
			<definition>Notes on spectral class
	<footnote footnoteId="???"><para>number=6</para>
			<para>e: emission lines
          p: peculiar spectra
          w: weak spectra lines
          c: evaluation of spectral class on the basis of known index of colour
          m: spectra of multiple system component
          l: luminosity class is estimated by the diagram "colour-luminosity"</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>l_Mass</name>
			<definition>Limit flag on Mass</definition>
			<units>---</units></field>
		<field>
			<name>Mass</name>
			<definition>Mass</definition>
			<units>solMass</units></field>
		<field>
			<name>n_Mass</name>
			<definition>Notes to Mass
	<footnote footnoteId="???"><para>number=7</para>
			<para>t: estimated by the relation of 'mass-effective temperature'
          c: calculated by the analysis of the line-of-sight curve of spectral
               binary stars
          S: summarized mass of seen and unseen components
          d: calculated by direct methods of mass measurement.
          w: calculated for white dwarfs by mass-radii relation</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>l_Rad</name>
			<definition>Limit flag on Radius</definition>
			<units>---</units></field>
		<field>
			<name>Rad</name>
			<definition>Radius</definition>
			<units>solRad</units></field>
		<field>
			<name>n_Rad</name>
			<definition>Notes to Rad
	<footnote footnoteId="???"><para>number=8</para>
			<para>t: estimated by the radii-effective temperature relation
          w: calculated for white dwarfs by mass-radii relation
          r: calculated by (V-R)-radii relation
          d: calculated by direct methods of radii measurement
----------------------------------------------------------------------------
References:
   1. Zakhozhaj V.A.                           =1979VKha...190...14...52Z
   2. Zakhozhaj V.A.                           =1982VKha...232...17...64Z
   3. Zakhozhaj V.A. 1987, Ph.D.Thesis, Leningrad.
   4. Zakhozhaj V.A.                           =1994KFNT...10b..68Z
   5. Zakhozhaj V.A. et al.                    =1994KFNT...10b..74Z
   6. Zakhozhaj V.A. 1995, Astron. Astrophys. Transact. (Moscow), 7, 167
   7. Zakhozhaj V.A., Shaparenko E.F.          =1996KFNT...12b..20Z
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Veta Avedisova</lastName>
				<affiliation>INASAN</affiliation></creator>
	<date>
		<year>1998</year><month>Aug</month><day>23</day></date></ingest>
		</history>
	<identifier>V_101.xml</identifier></dataset>
