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<ri:Resource created="2024-02-26T07:03:14Z" 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>Mind the Gap. I. Ha activity for M-Dwarfs</title><shortName>J/AJ/166/63</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/63</identifier><altIdentifier>doi:10.26093/cds/vizier.51660063</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jao W.-C.</name></creator><creator><name>Henry T.J.</name></creator><creator><name>White R.J.</name></creator><creator><name>Nisak A.H.</name></creator><creator><name>Hubbard-James H.-S.,Paredes L.A.</name></creator><creator><name>Lewis V.B.J.</name></creator><date role="Updated">2024-11-06T20:18:55Z</date><date role="Created">2024-02-26T07:03:14Z</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>m-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>proper-motions</subject><subject>trigonometric-parallax</subject><subject>radial-velocity</subject><description>Since identifying the gap in the H-R Diagram (HRD) marking the transition between partially and fully-convective interiors, a unique type of slowly pulsating M-dwarf has been proposed. These unstable M-dwarfs provide new laboratories in which to understand how changing interior structures can produce potentially observable activity at the surface. In this work, we report the results of the largest high-resolution spectroscopic H{alpha} emission survey to date spanning this transition region, including 480 M-dwarfs observed using the CHIRON spectrograph at CTIO/SMARTS 1.5m. We find that M dwarfs with H{alpha} in emission are almost entirely found 0-0.5mag above the top edge of the gap in the HRD, whereas effectively no stars in and below the gap show emission. Thus, the top edge of the gap marks a relatively sharp activity transition, and there is no anomalous H{alpha} activity for stars in the gap. We also identify a new region at 10.3&lt;MG&lt;10.8 on the main sequence where fewer M-dwarfs exhibit H{alpha} emission compared to M dwarfs above and below this magnitude range. Careful evaluation of the results in the literature indicates that (1) rotation and H{alpha} activity distributions on the main-sequence are closely related, and (2) fewer stars in this absolute magnitude range rotate in less than ~13days than populations surrounding this region. This result suggests that the most massive fully-convective stars lose their angular momentum faster than both partially convective stars and less massive fully-convective stars.</description><source format="bibcode">2023AJ....166...63J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/63</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/198">III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/806">J/AJ/113/806 : M-Subdwarfs (Gizis 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/3356">J/AJ/123/3356 : Palomar/MSU nearby star spectro survey. III. (Gizis+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/390/545">J/MNRAS/390/545 : Magnetic field &amp; velocity of early M dwarfs (Donati+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/785">J/AJ/135/785 : SDSS-DR5 low-mass star spectroscopic sample (West+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/97">J/AJ/141/97 : SDSS DR7 M dwarfs (West+, 2011)</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/ApJ/795/161">J/ApJ/795/161 : Activity &amp; rotation in Praesepe &amp; Hyades (Douglas+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/81">J/ApJ/788/81 : BANYAN III. 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(Paredes+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/916/77">J/ApJ/916/77 : K2 rot periods for SDSS &amp; Gaia Mdwarfs (Popinchalk+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/253/19">J/ApJS/253/19 : Halpha and other EWs of LAMOST M-type stars (Zhang+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/257">J/AJ/163/257 : Properties of 125 Mdwarfs in southern CVZ (Anthony+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/164/251">J/AJ/164/251 : ZTF measured rotational per of 40553 M-G-dwarfs (Lu+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/278">J/AJ/163/278 : Stellar populations in IC 2602 and IC 2391 (Nisak+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/662/A41">J/A+A/662/A41 : Magnetic fields in 292 M dwarfs. 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46039 46097 46100 46112 46154 46170 46173 46177 46189 46215-46216 46236 46276 46278 46287-46288 46299 46305 46314 46318 46323 46325 46345 46361 46364 46370 46379 46381 46396 46418 46425 46434 46445 46454 46456 46476 46495 46497 46504 46511 46518-46520 46523 46528 46530-46531 46534 46540 46542 46549 46565 46575 46581 46621 46628 46637 46640 46643 46651 46661 46665 46671 46673 46687-46688 46698 46702 46709 46712 46718 46720 46723 46736 46755 46767 46771 46783 46799 46807-46808 46824 46840-46841 46851 46885 46900 46910 46913-46914 46939 46942 46952 46985-46986 46993-46994 47009 47020 47039 47055 47067-47068 47086 47089-47090 47195 47217 47219 47298 47327 47367 47433 47452 47732 47953 48154 48181 48194 48196 48210 48235 48238 48242 48265 48390 48417 48436 48447 48493-48494 48529 48534 48566 48592 48597 48628 48934 48957 48970 48991 49016</spatial><spectral>1.9867573869263685e-19 3.916500758235022e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/166/63?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/166/63/table1</name><description>Selected M-dwarf targets close to the Gap</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>Obs</name><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></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>Gaia</name><description>Gaia EDR3 identifier</description><ucd>meta.id;meta.main</ucd><flag>primary</flag></column><column><name>RAICRS</name><description>[0/360] Right Ascension (ICRS at Epoch=2016)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEICRS</name><description>[-86/87] Declination (ICRS at Epoch=2016)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>plx</name><description>[10/220] Gaia EDR3 parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmRA</name><description>[-1222/1047] Gaia EDR3 proper motion in RA</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmDE</name><description>[-1666/796] Gaia EDR3 proper motion in DE</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RUWE</name><description>[0.79/1.4] Gaia EDR3 Renormalised Unit Weight Error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gmag</name><description>[8.03/15] Gaia EDR3 G-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPmag</name><description>[9.39/17] Gaia EDR3 BP-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPmag</name><description>[6.87/14] Gaia EDR3 RP-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/166/63/table4</name><description>Results</description><column><name>Gaia</name><description>Gaia EDR3 identifier</description><ucd>meta.id;meta.main</ucd></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>objID</name><description>Short Name used in this work</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>RAICRS</name><description>[0/23] Hour of Right Ascension (ICRS at Epoch=2016)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEICRS</name><description>Degree of Declination (ICRS at Epoch=2016)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>plx</name><description>[13.8/202] Gaia EDR3 parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RUWE</name><description>[0.79/1.4] Gaia EDR3 Renormalised Unit Weight Error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gmag</name><description>[8.2/14] Gaia EDR3 G-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BP-RP</name><description>[2.4/2.6] Gaia EDR3 BP-RP color</description><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NN</name><description>[0/10] Number of neighbors</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nvisit</name><description>[1/3] Number of observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>decker</name><description>Spectra were taken with CHIRON in fiber or slicer mode</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Epoch</name><description>[2018/2023] Epoch or RVel, years</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Act</name><description>[AE] H{alpha} profile, A=absorption; E=emission</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RVel</name><description>[-139/104] Radial velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[0.01/15] Uncertainty in RVel</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vsini</name><description>[10.1/21.3]? Projected rotational velocity</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_vsini</name><description>[0.9/2]? Uncertainty in vsini</description><unit>km/s</unit><ucd>stat.error;phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW</name><description>[-6.28/0.89] Equivalent width, Angstroms</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_EW</name><description>[0.01/0.2] Uncertainty in EW</description><unit>0.1nm</unit><ucd>stat.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CaH1</name><description>[0.15/1.16] CaH1 index</description><ucd>meta.code;spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>binflag</name><description>Binary flag, 1=possible binary</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>