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<ri:Resource created="2025-02-05T08:49:02Z" status="active" updated="2026-03-03T20:01:14Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>X-ray activity of nearby G-, K-, and M-type stars</title><shortName>J/A+A/694/A93</shortName><identifier>ivo://CDS.VizieR/J/A+A/694/A93</identifier><altIdentifier>doi:10.26093/cds/vizier.36940093</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhu E.</name></creator><creator><name>Preibisch T.</name></creator><date role="Updated">2026-03-03T20:01:14Z</date><date role="Created">2025-02-05T08:49:02Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>x-ray-sources</subject><subject>m-stars</subject><description>The intense X-ray and UV emission of some active M stars has raised questions about the habitability of planets around M-type stars. We aim to determine the unbiased distribution of X-ray luminosities in complete, volume-limited samples of nearby M dwarfs, and compare them to those of K and G dwarfs. We have constructed volume-complete samples of 205 M stars with spectral type &lt;=M6 within 10pc from the Sun, 129 K stars within 16pc, and 107 G stars within 20pc. We use X-ray data from Chandra, XMM-Newton, eROSITA, and ROSAT to obtain the X-ray luminosities of the stars. Our samples reach an X-ray detection completeness of 85%, 86%, and 80% for M, K, and G stars. The fractional X-ray luminosities, log(LX/Lbol), of the M stars show a bimodal distribution with one peak at around ~5, mostly contributed by early M stars (M0-M4), and another peak around ~3.5, contributed mainly by M4-M6 stars. The comparison of the different spectral classes shows that 63% of all M stars in our sample (80% of the M stars with spectral type &lt;M4) have LX/Lbol values that are within the central 80% quantile of the distribution function for G stars. 55% of all M stars in our sample (and 72% of the M stars with spectral type &lt;M4) have LX/Lbol less than 10 times the solar value. The X-ray activity levels of the majority (~&gt;60%) of nearby M dwarfs no later than M6 are actually not higher than the typical (80% quantile) levels for G-type stars. The X-ray irradiation of habitable-zone planets around these stars should therefore not present a specific problem for their habitability.</description><source format="bibcode">2025A&amp;A...694A..93Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/694/A93</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/670/A19">J/A+A/670/A19 : Fifth Catalogue of Nearby Stars (CNS5) (Golovin+, 2023)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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X-ray luminosity according to eROSITA</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXeROSITA</name><description>? Upper error of LXeROSITA</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXeROSITA</name><description>? Lower error of LXeROSITA</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXeROSITA</name><description>[0/1]? Flag for LXeROSITA as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BandLXeROSITA</name><description>Energy band of LXeROSITA</description><unit>keV</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>r_LXeROSITA</name><description>Reference of LXeROSITA</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LXROSAT</name><description>? X-ray luminosity according to ROSAT</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXROSAT</name><description>? Upper error of LXROSAT</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXROSAT</name><description>? Lower error of LXROSAT</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXROSAT</name><description>[0/1]? Flag for LXROSAT as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BandLXROSAT</name><description>Energy band of LXROSAT</description><unit>keV</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>InstLXROSAT</name><description>Camera of ROSAT used</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>r_LXROSAT</name><description>Reference of LXROSAT</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LXother</name><description>? X-ray luminosity according to other telescopes (Chandra or XMM-Newton)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXother</name><description>? Upper error of LXother</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXother</name><description>? Lower error of LXother</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXother</name><description>[0/1]? Flag for LXother as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BandLXother</name><description>Energy band of LXother</description><unit>keV</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>InstLXother</name><description>Camera of other telescopes used</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>r_LXother</name><description>Reference of LXother</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LXfinal</name><description>? X-ray luminosity used in the analysis, converted to ROSAT energy band</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXfinal</name><description>? Upper error of LXfinal</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXfinal</name><description>? Lower error of LXfinal</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXfinal</name><description>[0/1]? Flag for LXfinal as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lbol</name><description>? Bolometric luminosity</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_Lbol</name><description>Reference of _bol</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LX/Lbol</name><description>? LX/Lbol used in the final analysis</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LX/Lbol</name><description>? Upper error of LX/Lbol</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LX/Lbol</name><description>? Lower error of LX/Lbol</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/A+A/694/A93/m-xray</name><description>X-ray data of nearby M stars (table F1)</description><column><name>DEJ2000</name><description>Declination (J2000) (Gaia DR3)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>fGaia</name><description>[0/1] Flag for stars with peculiar Gaia colours</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SpType</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>r_SpType</name><description>Reference of SpType</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CNS5</name><description>? Designation in CNS5</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GJ</name><description>? Gliese-Jahreiss number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>OName</name><description>Name of stars that do not have CNS5 and GJ</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>Comp</name><description>Component in a multiple system</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000) (Gaia DR3)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>GSpType</name><description>Spectral type according to M_G_ which is different from literature SpType</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Distance</name><description>Gaia DR3 distance to the Sun</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LXeROSITA</name><description>? X-ray luminosity according to eROSITA</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXeROSITA</name><description>? Upper error of LXeROSITA</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXeROSITA</name><description>? Lower error of LXeROSITA</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXeROSITA</name><description>[0/1]? Flag for LXeROSITA as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BandLXeROSITA</name><description>Energy band of LXeROSITA</description><unit>keV</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>r_LXeROSITA</name><description>Reference of LXeROSITA</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LXROSAT</name><description>? X-ray luminosity according to ROSAT</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXROSAT</name><description>? Upper error of LXROSAT</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXROSAT</name><description>? Lower error of LXROSAT</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXROSAT</name><description>[0/1]? Flag for LXROSAT as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BandLXROSAT</name><description>Energy band of LXROSAT</description><unit>keV</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>InstLXROSAT</name><description>Camera of ROSAT used</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>r_LXROSAT</name><description>Reference of LXROSAT</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LXother</name><description>? X-ray luminosity according to other telescopes (Chandra or XMM-Newton)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXother</name><description>? Upper error of LXother</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXother</name><description>? Lower error of LXother</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXother</name><description>[0/1]? Flag for LXother as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BandLXother</name><description>Energy band of LXother</description><unit>keV</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>InstLXother</name><description>Camera of other telescopes used</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>r_LXother</name><description>Reference of LXother</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LXfinal</name><description>? X-ray luminosity used in the analysis, converted to ROSAT energy band</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LXfinal</name><description>? Upper error of LXfinal</description><unit>1e-07W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LXfinal</name><description>? Lower error of LXfinal</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_LXfinal</name><description>[0/1]? Flag for LXfinal as upper limit value (1 = yes)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lbol</name><description>? Bolometric luminosity</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_Lbol</name><description>Reference of _bol</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LX/Lbol</name><description>? LX/Lbol used in the final analysis</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_LX/Lbol</name><description>? Upper error of LX/Lbol</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LX/Lbol</name><description>? Lower error of LX/Lbol</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>