<?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>High resolution spectra of Very Low-Mass Stars</title>
	<altname type="ADC">J/MNRAS/301/1031</altname>
		<altname type="CDS">J/MNRAS/301/1031</altname>
		<altname type="brief">High resolution spectra of VLM stars</altname>
	<reference>
		<source>
<journal>
	<title>High resolution spectra of Very Low-Mass Stars</title>
	<author>
			<initial>C</initial>
			<initial>G</initial>
			<lastName>Tinney</lastName></author>
	<author>
			<initial>I</initial>
			<initial>N</initial>
			<lastName>Reid</lastName></author>
	<name>Mon. Not. R. Astron. Soc.</name>
	<volume>301</volume>
	<pageno>1031</pageno>
		<date>
			<year>1998</year></date>
	<bibcode>1998MNRAS.301.1031T</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Spectroscopy.html">Spectroscopy</keyword>
			<keyword xlink:href="Stars_dwarfs.html">Stars, dwarfs</keyword>
			<keyword xlink:href="Stars_late-type.html">Stars, late-type</keyword></keywords>
	<descriptions>
				<description>
				<para>
   A high resolution optical spectral atlas for three very low-mass
   stars are provided, along with a high resolution observation of
   an atmospheric absorption calibrator. This is the data used to
   produce Figures 4-9 in the paper.</para><para>   These data were acquired with CASPEC on the ESO3.6m telescope.
   The FWHM resolution is 16km/s (eg. 0.043nm at 800nm), at a dispersion
   of 9km/s. Incomplete wavelength coverage produces inter-order gaps
   at wavelengths longer than 804.5nm.</para></description>
                        <details>
	<astroObjects>
		
			<astroObject><name>VB 8</name><name>LHS 429</name><name>Gl 644 C      (vb8.dat)</name><position><ra>16 55 35.7</ra><dec>-08 23 36</dec></position></astroObject>
			<astroObject><name>LHS 2065</name><name>LP 666-9            (lhs2065.dat)</name><position><ra>08 53 36</ra><dec>-03 29 30</dec></position></astroObject>
			<astroObject><name>LP 944-20                      (lp944-20.dat)</name><position><ra>03 39 34.6</ra><dec>-35 25 51</dec></position></astroObject>
			<astroObject><name>mu Col</name><name>HR 1996</name><name>HD 38666  (mucol.dat)</name><position><ra>05 45 59.9</ra><dec>-32 18 23</dec></position></astroObject></astroObjects></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="vb8.dat">
	<title>Spectrum for VB8</title></tableLink>
				<tableLink xlink:href="lhs2065.dat">
	<title>Spectrum for LHS2065</title></tableLink>
				<tableLink xlink:href="lp944-20.dat">
	<title>Spectrum for LP944-20</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Lambda</name>
			<definition>Central wavelength of the flux bin</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Fnu</name>
			<definition>Data in interorder gaps has value 0.0</definition>
			<units>mJy</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="mucol.dat">
	<title>Atmospheric Spectrum for Mu Columbae</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Lambda</name>
			<definition>Central wavelength of the flux bin</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Fnu</name>
			<definition>Data in interorder gaps has value 0.0
	<footnote>
			<para>
  mJy which have been normalised to value 1.0
  in the continuum of the atmospheric standard star
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>C.G. Tinney</lastName>
				<affiliation>AAO</affiliation></creator>
	<date>
		<year>1999</year><month>Feb</month><day>04</day></date></ingest>
		</history>
	<identifier>J_MNRAS_301_1031.xml</identifier></dataset>
