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<ri:Resource created="2020-08-13T09:59:51Z" status="active" updated="2025-06-13T15:25:00Z" 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>HAZMAT. V. UV and X-ray evolution of K stars</title><shortName>J/ApJ/872/17</shortName><identifier>ivo://CDS.VizieR/J/ApJ/872/17</identifier><altIdentifier>doi:10.26093/cds/vizier.18720017</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Richey-Yowell T.</name></creator><creator><name>Shkolnik E.L.</name></creator><creator><name>Schneider A.C.</name></creator><creator><name>Osby E.</name></creator><creator><name>Barman T.,Meadows V.S.</name></creator><date role="Updated">2021-09-07T13:10:14Z</date><date role="Created">2020-08-13T09:59:51Z</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>k-stars</subject><subject>ultraviolet-photometry</subject><subject>x-ray-sources</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>stellar-distance</subject><description>Knowing the high-energy radiation environment of a star over a planet's formation and evolutionary period is critical in determining if that planet is potentially habitable and if any biosignatures could be detected, as UV radiation can severely change or destroy a planet's atmosphere. Current efforts for finding a potentially habitable planet are focused on M stars, yet K stars may offer more habitable conditions due to decreased stellar activity and more distant and wider habitable zones (HZs). While M star activity evolution has been observed photometrically and spectroscopically, there has been no dedicated investigation of K star UV evolution. We present the first comprehensive study of the near-UV, far-UV, and X-ray evolution of K stars. We used members of young moving groups and clusters ranging in age from 10 to 625Myr combined with field stars and their archived GALEX UV and ROSAT X-ray data to determine how the UV and X-ray radiation evolve. We find that the UV and X-ray flux incident on an HZ planet is 5-50 times lower than that of HZ planets around early-M stars and 50-1000 times lower than those around late-M stars, due to both an intrinsic decrease in K dwarf stellar activity occurring earlier than for M dwarfs and the more distant location of the K dwarf HZ.</description><source format="bibcode">2019ApJ...872...17R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/872/17</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/IX/10">IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Revised catalog of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/331/81">J/A+A/331/81 : Hyades membership (Perryman+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/328/45">J/MNRAS/328/45 : Late-type stars members of young groups (Montes+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2340">J/AJ/134/2340 : Praesepe &amp; Coma Berenices cluster memberships (Kraus+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/761/166">J/ApJ/761/166 : Terrestrial exoplanet atmospheres. 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(Hu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/422/2024">J/MNRAS/422/2024 : X-ray-age relation &amp; exoplanet evaporation (Jackson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/559/A43">J/A+A/559/A43 : Pan-STARRS1 (PS1) obs. of the Hyades (Goldman+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/762/88">J/ApJ/762/88 : Young stellar kinematic group cand. members (Malo+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors &amp; temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/2063">J/MNRAS/431/2063 : UV/X-ray activity of M dwarfs within 10pc (Stelzer+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/146">J/AJ/147/146 : Spectroscopy of Tuc-Hor candidate members (Kraus+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/64">J/AJ/148/64 : HAZMAT. I. FUV &amp; NUV in early M stars (Shkolnik+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/593">J/MNRAS/454/593 : Young moving groups in solar neighbourhood (Bell+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/588/A103">J/A+A/588/A103 : 2nd ROSAT all-sky survey (2RXS) source cat. (Boller+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/67">J/AJ/154/67 : HAZMAT. II. Low-mass stars with GALEX UV obs. (Miles+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/69">J/AJ/154/69 : ACRONYM II. {beta} Pictoris Moving Group (Shkolnik+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/2">J/ApJS/239/2 : Simulated exoplanets from TESS targets (Barclay+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/122">J/AJ/155/122 : HAZMAT. III. Low-mass stars GALEX photom. 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