<?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>Stellar effective temperatures and angular diameters determined by the infrared
flux method (IRFM): revisions using improved Kurucz LTE stellar atmospheres</title>
	<altname type="ADC">J/A+A/282/899</altname>
		<altname type="CDS">J/A+A/282/899</altname>
		<altname type="brief">Stellar effective temperatures and angular</altname>
	<reference>
		<source>
<journal>
	<title>Stellar effective temperatures and angular diameters determined by the infrared
flux method (IRFM): revisions using improved Kurucz LTE stellar atmospheres</title>
	<author>
			<initial>D</initial>
			<initial>E</initial>
			<lastName>Blackwell</lastName></author>
	<author>
			<initial>A</initial>
			<initial>E</initial>
			<lastName>Lynas-Gray</lastName></author>
	<name>Astron. Astrophys.</name>
	<volume>282</volume>
	<pageno>899</pageno>
		<date>
			<year>1994</year></date>
	<bibcode>1994A&amp;A...282..899B</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Effective_temperatures.html">Effective temperatures</keyword>
			<keyword xlink:href="Stars_diameters.html">Stars, diameters</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="stars_atmospheres.html">stars: atmospheres</keyword>
			<keyword xlink:href="stars_fundamental_parameters.html">stars: fundamental parameters</keyword></keywords>
	<descriptions>
			<description>
				<heading>*** No Description Available ***</heading></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Values of Log R as a function of temperature,
                                  wavelength and surface gravity</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>log.g</name>
			<definition>Surface gravity</definition>
			<units>cm/s2</units></field>
		<field>
			<name>Teff</name>
			<definition>Effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>LogR1</name>
			<definition>Ratio of integrated flux to
                                   monochromatic flux lambda 1.2467 um</definition>
			<units>---</units></field>
		<field>
			<name>LogR2</name>
			<definition>Ratio of integrated flux to
                                   monochromatic flux lambda 2.2135 um</definition>
			<units>---</units></field>
		<field>
			<name>LogR3</name>
			<definition>Ratio of integrated flux to
                                   monochromatic flux lambda 3.7825 um</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Effect on determined effective temperatures of
                                  using Kurucz (1992) model atmospheres instead
                                  of MARCS atmospheres</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Teff</name>
			<definition>Effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>TcJ</name>
			<definition>Temperature change for use of filter J</definition>
			<units>K</units></field>
		<field>
			<name>TcK</name>
			<definition>Temperature change for use of filter K</definition>
			<units>K</units></field>
		<field>
			<name>TcL</name>
			<definition>Temperature change for use of filter L</definition>
			<units>K</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3">
	<title>Effect on determined temperatures at J, K, L
                                  for a change in surface gravity</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Filter</name>
			<definition>Filter used</definition>
			<units>---</units></field>
		<field>
			<name>Teff</name>
			<definition>Effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>Tc2</name>
			<definition>Temperature change for log g=2</definition>
			<units>K</units></field>
		<field>
			<name>Tc3</name>
			<definition>Temperature change for log g=3</definition>
			<units>K</units></field>
		<field>
			<name>Tc3</name>
			<definition>Temperature change for log g=4</definition>
			<units>K</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>Effect of A(V) on effective temperatures</title></tableLink>
				<tableLink xlink:href="table7">
	<title>Effect of A(V) on the integrated flux</title></tableLink>
				<tableLink xlink:href="table13">
	<title>Effect of A(V) on angular diameters</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Teff</name>
			<definition>Effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>CF5</name>
			<definition>Correction factors for A(V)=0.05m</definition>
			<units>---</units></field>
		<field>
			<name>CF10</name>
			<definition>Correction factors for A(V)=0.10m</definition>
			<units>---</units></field>
		<field>
			<name>CF15</name>
			<definition>Correction factors for A(V)=0.15m</definition>
			<units>---</units></field>
		<field>
			<name>CF20</name>
			<definition>Correction factors for A(V)=0.20m</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table5">
	<title>Effect of a one per cent decrease in flux at
                                  J, K, L wavelengths on temperatures</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Teff</name>
			<definition>Effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>TcJ</name>
			<definition>Temperature change at J wavelength</definition>
			<units>K</units></field>
		<field>
			<name>TcK</name>
			<definition>Temperature change at K wavelength</definition>
			<units>K</units></field>
		<field>
			<name>TcL</name>
			<definition>Temperature change at L wavelength</definition>
			<units>K</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table6">
	<title>Parameters of selected stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>BS</name>
			<definition>BS (Bright Star catalogue) number</definition>
			<units>---</units></field>
		<field>
			<name>n_BS</name>
			<definition>When *, known spectroscopic binary</definition>
			<units>---</units></field>
		<field>
			<name>SC</name>
			<definition>Spectral class</definition>
			<units>---</units></field>
		<field>
			<name>A(V)</name>
			<definition>Interstellar extinction</definition>
			<units>mag</units></field>
		<field>
			<name>V</name>
			<definition>Visual magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V color</definition>
			<units>mag</units></field>
		<field>
			<name>V-K</name>
			<definition>V-K color</definition>
			<units>mag</units></field>
		<field>
			<name>log.g</name>
			<definition>Surface gravity</definition>
			<units>cm/s2</units></field>
		<field>
			<name>Fe/H</name>
			<definition>Metallicity</definition>
			<units>---</units></field>
		<field>
			<name>FT</name>
			<definition>Total flux</definition>
			<units>10-9W/m2</units></field>
		<field>
			<name>Teff</name>
			<definition>Effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>D</name>
			<definition>Angular diameter</definition>
			<units>mas</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table8">
	<title>Coefficients A,B,C in the relation
                                  temperature = A+B*(V-K)+C*(V-K)**2</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Type</name>
			<definition>Kind of star
	<footnote footnoteId="???"><para>number=</para>
			<para>  Temperature = A + B(V-K) + C(V-K)^2
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>A</name>
			<definition>Coefficient A
	<footnote footnoteId="???"><para>number=</para>
			<para>  Temperature = A + B(V-K) + C(V-K)^2
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>B</name>
			<definition>Coefficient B
	<footnote footnoteId="???"><para>number=</para>
			<para>  Temperature = A + B(V-K) + C(V-K)^2
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>C</name>
			<definition>Coefficient C
	<footnote footnoteId="???"><para>number=</para>
			<para>  Temperature = A + B(V-K) + C(V-K)^2
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table9">
	<title>Comparison between determined temperatures and
                                  calculated temperatures for stars which as not
                                  been detected as spectroscopic binaries</title></tableLink>
				<tableLink xlink:href="table10">
	<title>Comparison between determined temperatures and
                                  calculated temperatures for known
                                  spectroscopic binaries</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>BS</name>
			<definition>BS (Bright Star catalogue) number</definition>
			<units>---</units></field>
		<field>
			<name>Tm</name>
			<definition>Measured temperature</definition>
			<units>K</units></field>
		<field>
			<name>Tc</name>
			<definition>Calculated temperature
	<footnote footnoteId="???"><para>number=1</para>
			<para>
       For table9, temperature = 8906 - 2625*(V-K) + 363.2*(V-K)^2
                   where V-K has been corrected for interstellar extinction.
                   The stars have not been detected to be spectroscopic binaries


       For table10, temperature = 8825 - 2548*(V-K) + 343.9*(V-K)^2,
                    where V-K has been corrected for interstellar extinction.
                    The stars are known spectroscopic binaries
</para></footnote></definition>
			<units>K</units></field>
		<field>
			<name>R</name>
			<definition>Residual (measured - calculated temperature)</definition>
			<units>%</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table11">
	<title>Comparison of IRFM effective temperatures with
                                  'adopted' temperatures of Bell and Gustafsson</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>BS</name>
			<definition>BS (Bright Star catalogue) number</definition>
			<units>---</units></field>
		<field>
			<name>Tbg</name>
			<definition>Adopted temperature of Bell &amp; Gustafsson
	<footnote footnoteId="???"><para>number=1</para>
			<para>Bell R.A., Gustafsson B., 1989, MNRAS, 236, 653
</para></footnote></definition>
			<units>K</units></field>
		<field>
			<name>Tirfm</name>
			<definition>IRFM (Infrared Flux Method) effective
                                    temperature</definition>
			<units>K</units></field>
		<field>
			<name>Tirfm-Tbg</name>
			<definition>Temperature differences Tirfm - Tbg</definition>
			<units>%</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table12">
	<title>Relation between temperatures determined by
                                  Ridgway et al. and present IRFM temperatures</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>V-K</name>
			<definition>V-K color</definition>
			<units>mag</units></field>
		<field>
			<name>Tirfm</name>
			<definition>IRFM effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>Tr</name>
			<definition>Adopted temperature of Ridgway et al.
	<footnote footnoteId="???"><para>number=1</para>
			<para>Ridgway S.T. et al., 1980, ApJ, 235, 126
</para></footnote></definition>
			<units>K</units></field>
		<field>
			<name>Tirfm-Tr</name>
			<definition>Temperature differences Tirfm - Tr</definition>
			<units>K</units></field>
		<field>
			<name>Tirfm-Tr</name>
			<definition>Temperature differences Tirfm - Tr percent</definition>
			<units>%</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table14">
	<title>Comparison between angular diameters determined
                                  by Michelson interferometry and
                                  present IRFM determinations</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>BS</name>
			<definition>BS (Bright Star catalogue) number</definition>
			<units>---</units></field>
		<field>
			<name>ADi</name>
			<definition>IRFM angular diameter</definition>
			<units>---</units></field>
		<field>
			<name>ADm</name>
			<definition>Michelson interferometry angular diameter
	<footnote footnoteId="???"><para>number=1</para>
			<para>Mozurkewich D. et al., 1991, AJ, 101, 2207
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>ADi-ADm</name>
			<definition>Angular diameter difference IRFM-Michelson</definition>
			<units>%</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Mar</month><day>14</day></date></ingest>
		</history>
	<identifier>J_A+A_282_899.xml</identifier></dataset>
