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<ri:Resource created="2023-09-19T06:27:28Z" 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>Tull RVels, rotation periods and Inclinations</title><shortName>J/AJ/165/164</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/164</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bowler B.P.</name></creator><creator><name>Tran Q.H.</name></creator><creator><name>Zhang Z.</name></creator><creator><name>Morgan M.</name></creator><creator><name>Ashok K.B.</name></creator><creator><name>Blunt S.,Bryan M.L.</name></creator><creator><name>Evans A.E.</name></creator><creator><name>Franson K.</name></creator><creator><name>Huber D.</name></creator><creator><name>Nagpal V.</name></creator><creator><name>Wu Y.-L.,Zhou Y.</name></creator><date role="Updated">2024-07-09T07:43:47Z</date><date role="Created">2023-09-19T06:27:28Z</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>brown-dwarfs</subject><subject>exoplanets</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><subject>radial-velocity</subject><description>The orientation between a star's spin axis and a planet's orbital plane provides valuable information about the system's formation and dynamical history. For non-transiting planets at wide separations, true stellar obliquities are challenging to measure, but lower limits on spin-orbit orientations can be determined from the difference between the inclination of the star's rotational axis and the companion's orbital plane ({Delta}i). We present results of a uniform analysis of rotation periods, stellar inclinations, and obliquities of cool stars (SpT&gt;~F5) hosting directly imaged planets and brown dwarf companions. As part of this effort, we have acquired new vsini* values for 22 host stars with the high-resolution Tull spectrograph at the Harlan J. Smith telescope. Altogether our sample contains 62 host stars with rotation periods, most of which are newly measured using light curves from the Transiting Exoplanet Survey Satellite. Among these, 53 stars have inclinations determined from projected rotational and equatorial velocities, and 21 stars predominantly hosting brown dwarfs have constraints on {Delta}i. Eleven of these (52_-11_^+10^% of the sample) are likely misaligned, while the remaining 10 host stars are consistent with spin- orbit alignment. As an ensemble, the minimum obliquity distribution between 10 and 250au is more consistent with a mixture of isotropic and aligned systems than either extreme scenario alone-pointing to direct cloud collapse, formation within disks bearing primordial alignments and misalignments, or architectures processed by dynamical evolution. This contrasts with stars hosting directly imaged planets, which show a preference for low obliquities. These results reinforce an emerging distinction between the orbits of long- period brown dwarfs and giant planets in terms of their stellar obliquities and orbital eccentricities.</description><source format="bibcode">2023AJ....165..164B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/164</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/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/117">V/117 : Geneva-Copenhagen Survey of Solar neighbourhood (Holmberg+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/135">J/ApJS/99/135 : Rotation and Spectral Peculiarities (Abt+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/457/L99">J/ApJ/457/L99 : 25yr CaII-HK observations F-K nearby stars (Baliunas+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/508/397">J/ApJ/508/397 : H-band Spectral Standards (Meyer+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/140/29">J/A+AS/140/29 : Photo monitoring of 47 late-type stars (Strassmeier+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/384/491">J/A+A/384/491 : Fast-rotating nearby solartype stars I (Cutispoto+, 2002-03)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/275">J/A+AS/142/275 : Stellar activity of late-type stars (Strassmeier+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/393/897">J/A+A/393/897 : Rotational velocities of A-type stars II. 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