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<ri:Resource created="2015-07-09T13:58:13Z" 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>25yr CaII-HK observations of F-K nearby stars</title><shortName>J/ApJ/457/L99</shortName><identifier>ivo://CDS.VizieR/J/ApJ/457/L99</identifier><altIdentifier>doi:10.26093/cds/vizier.14579099</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Baliunas S.</name></creator><creator><name>Sokoloff D.</name></creator><creator><name>Soon W.</name></creator><date role="Updated">2018-05-28T16:03:55Z</date><date role="Created">2015-07-09T13:58:13Z</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>g-stars</subject><subject>visible-astronomy</subject><subject>narrow-band-photometry</subject><description>We find a significant correlation between the magnetic and rotational moments for a sample of 112 lower main-sequence stars. The rotational moment is calculated from measurements of the rotation period in most of the stars (not from the projected rotational velocity inferred from Doppler broadening). The magnetic moment is computed from a database of homogeneous measurements of the mean level of Ca II H and K emission fluxes sampled for most of the stars over an interval of 25yr. The slope connecting the logarithm of the magnetic moment and the logarithm of the rotational moment is about +0.5-0.6, with a Pearson correlation coefficient of about +0.9. The scatter of points from the mean relation has a component that is natural and caused by decade-long surface variability.</description><source format="bibcode">1996ApJ...457L..99B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/457/L99</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/III/159">III/159 : Ca II H and K Measurements Made at MWO (Duncan+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/552/A114">J/A+A/552/A114 : Sun chromospheric CaII-HK emission (Shapiro+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/552/A27">J/A+A/552/A27 : Stellar activity and kinematics of FGK stars (Murgas+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/L8">J/A+A/551/L8 : Chromospheric activity of field stars (Pace, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/547/A106">J/A+A/547/A106 : Li abundances in the FGK dwarfs (Mishenina+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/531/A8">J/A+A/531/A8 : Activity indexes and velocities for 890 stars (Jenkins+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/88/1217">J/AZh/88/1217 : Solar-like activity of low-mass stars (Kasova+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/48">J/ApJ/743/48 : Stellar rotation periods &amp; X-ray luminosities (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/725/875">J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/520/A79">J/A+A/520/A79 : FGK stars chromospheric activity (Martinez-Arnaiz+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/1099">J/A+A/493/1099 : CaII HK emission in rapidly rotating stars (Schroeder+, 2009)</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/A+A/483/903">J/A+A/483/903 : Mt Wilson index for main sequence F-K stars (Buccino+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/469/309">J/A+A/469/309 : Chromospheric activity in late-type stars (Cincunegui+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2524">J/AJ/133/2524 : Spectra of young nearby stars (White+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/152/261">J/ApJS/152/261 : Chromospheric Ca II emission in nearby stars (Wright+, 2004)</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/A+AS/146/103">J/A+AS/146/103 : CaII H+K to CaII IRT echelle spectra (Montes+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/116/1922">J/AJ/116/1922 : CaII H and K filter photometry III. 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