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<ri:Resource created="2020-10-16T11:15:50Z" status="active" updated="2025-05-19T09:50:00Z" 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>J, Ks, NUV emission of 133 red giant stars</title><shortName>J/AJ/160/12</shortName><identifier>ivo://CDS.VizieR/J/AJ/160/12</identifier><altIdentifier>doi:10.26093/cds/vizier.51600012</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dixon D.</name></creator><creator><name>Tayar J.</name></creator><creator><name>Stassun K.G.</name></creator><date role="Updated">2022-09-26T06:40:57Z</date><date role="Created">2020-10-16T11:15:50Z</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>giant-stars</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>infrared-photometry</subject><description>Main-sequence stars exhibit a clear rotation-activity relationship, in which rapidly rotating stars drive strong chromospheric/coronal ultraviolet and X-ray emission. While the vast majority of red giant stars are inactive, a few percent exhibit strong ultraviolet emission. Here we use a sample of 133 red giant stars observed by Sloan Digital Sky Survey APOGEE and Galaxy Evolution Explorer to demonstrate an empirical relationship between near-UV (NUV) excess and rotational velocity (vsini). Beyond this simple relationship, we find that NUV excess also correlates with rotation period and with Rossby number in a manner that shares broadly similar trends to those found in M dwarfs, including activity saturation among rapid rotators. Our data also suggest that the most extremely rapidly rotating giants may exhibit so-called supersaturation, which could be caused by centrifugal stripping of these stars rotating at a high fraction of breakup speed. As an example application of our empirical rotation-activity relation, we demonstrate that the NUV emission observed from a recently reported system comprising a red giant with a black hole companion is fully consistent with arising from the rapidly rotating red giant in that system. Most fundamentally, our findings suggest a common origin of chromospheric activity in rotation and convection for cool stars from main sequence to red giant stages of evolution.</description><source format="bibcode">2020AJ....160...12D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/12</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/312">II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/139/433">J/A+AS/139/433 : RV and vsini of evolved stars (de Medeiros+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/397/147">J/A+A/397/147 : Activity-rotation relationship in stars (Pizzolato+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/1264">J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/1338">J/AJ/139/1338 : UV-selected stars in Tau and Upper Sco (Findeisen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/732/39">J/ApJ/732/39 : Rotational velocities of K giant stars (Carlberg+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/411/2099">J/MNRAS/411/2099 : Fast-rotating M-dwarf stars in NGC 2547 (Jeffries+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/48">J/ApJ/743/48 : Stars with rotation periods &amp; X-ray lum. (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/133">J/AJ/146/133 : Stellar param. from SDSS-III APOGEE DR10 (Meszaros+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/82">J/ApJ/807/82 : Rotational velocities of APOKASC red giants (Tayar+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for 15 APOGEE chem. elements (Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/1844">J/MNRAS/463/1844 : M dwarfs rotation-activity relation (Stelzer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/605/A111">J/A+A/605/A111 : Surface rotation of Kepler red giant stars (Ceillier+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/94">J/AJ/154/94 : APOGEE-2 data from DR16 (Majewski+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/259">J/AJ/154/259 : Fundamental param. of Tycho-2 &amp; TGAS stars (Stevens+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/612/A48">J/A+A/612/A48 : 4 oxygen-rich evolved stars NH3 spectra (Wong+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/16">J/ApJS/235/16 : UV emission of stars in LAMOST. 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