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<ri:Resource created="2023-01-23T08:59:05Z" 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>X-ray superflares from PMS stars in MYStIX &amp; SFiNCs</title><shortName>J/ApJ/916/32</shortName><identifier>ivo://CDS.VizieR/J/ApJ/916/32</identifier><altIdentifier>doi:10.26093/cds/vizier.19160032</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Getman K.V.</name></creator><creator><name>Feigelson E.D.</name></creator><date role="Updated">2023-08-16T15:05:30Z</date><date role="Created">2023-01-23T08:59:05Z</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>x-ray-sources</subject><subject>surveys</subject><subject>pre-main-sequence-stars</subject><subject>stellar-flares</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>star-forming-regions</subject><subject>infrared-sources</subject><description>Solar-type stars exhibit their highest levels of magnetic activity during their early convective pre-main-sequence (PMS) phase of evolution. The most powerful PMS flares, superflares and megaflares, have peak X-ray luminosities of log(L_X_)=30.5-34.0erg/s and total energies log(E_X_)=34-38erg. Among &gt;24000 X-ray-selected young (t&lt;~5Myr) members of 40 nearby star-forming regions from our earlier Chandra MYStIX and SFiNCs surveys, we identify and analyze a well-defined sample of 1086 X-ray superflares and megaflares, the largest sample ever studied. Most are considerably more powerful than optical/X-ray superflares detected on main-sequence stars. This study presents energy estimates of these X-ray flares and the properties of their host stars. These events are produced by young stars of all masses over evolutionary stages ranging from protostars to diskless stars, with the occurrence rate positively correlated with stellar mass. Flare properties are indistinguishable for disk- bearing and diskless stars indicating star-disk magnetic fields are not involved. A slope of {alpha}~2 in the flare energy distributions dN/dE_X_{propto}E_X_^-{alpha}^ is consistent with that of optical/X-ray flaring from older stars and the Sun. Megaflares (log(E_X_)&gt;36.2erg) from solar-mass stars have an occurrence rate of 1.7_-0.6_^+1.0^ flares/star/year and contribute at least 10%-20% to the total PMS X-ray energetics. These explosive events may have important astrophysical effects on protoplanetary disk photoevaporation, ionization of disk gas, production of spallogenic radionuclides in disk solids, and hydrodynamic escape of young planetary atmospheres. Our following paper details plasma and magnetic loop modeling of the &gt;50 brightest X-ray megaflares.</description><source format="bibcode">2021ApJ...916...32G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/916/32</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/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/341">II/341 : VPHAS+ DR2 survey (Drew+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/348">II/348 : VISTA Variable in the Via Lactea Survey DR2 (Minniti+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/156">VI/156 : M-dwarf Lum-Temp-Radius relationships (Morrell+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/160/319">J/ApJS/160/319 : COUP: observations and source lists (Getman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/474/495">J/A+A/474/495 : X-ray flares from Cygnus OB2 stars (Albacete Colombo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/169/353">J/ApJS/169/353 : Chandra sources in M17 (Broos+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/468/353">J/A+A/468/353 : XMM-Newton Extended Survey of Taurus (Guedel+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/492/277">J/A+A/492/277 : Analysis of Collinder 69 stars with VOSA (Bayo+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/688/418">J/ApJ/688/418 : X-ray flares in Orion young stars. 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Reddening, V-band (2)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age</name><description>[0.4/5]? Age (2)</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logTeff</name><description>[3.4/4.8]? log of surface effective temperature (2)</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logLbol</name><description>[-1.4/7]? log of bolometric luminosity (2)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mstar</name><description>[0.1/320.2]? Mass (2)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rstar</name><description>[0.9/31.4]? Radius (2)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>alpha</name><description>[-4.3/4.4]? IRAC SED slope (2)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Flag</name><description>Flag (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>MYStIX</name><description>Display data from Kuhn+ 2013, J/ApJS/209/27 and Broos+ 2013, J/ApJS/209/32</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SFiNCS</name><description>Display data from Getman+, 2017, J/ApJS/229/28</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Nf</name><description>Number of flares for this star (link to Table 3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/916/32/table3</name><description>MYStIX and SFiNCs F+R+D super-flares</description><column><name>ObsID</name><description>[1/9] Relative sequence number of the X-ray Chandra observation (G1) (1)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Exp</name><description>[11.8/154] Chandra ObsID Exposure</description><unit>ks</unit><ucd>time.expo</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Class</name><description>Flare class (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Nphot</name><description>[15/19891] Flare X-ray counts</description><unit>ct</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ME</name><description>[0.9/5.7] Flare median photon energy</description><unit>keV</unit><ucd>phys.energy;stat.median;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Region</name><description>Star forming region (See Table 1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>l_Dur</name><description>Limit flag on Dur</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Dur</name><description>[1.9/153.9] Flare duration</description><unit>ks</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_logLxpk</name><description>Limit flag on logLxpk</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logLxpk</name><description>[30.6/33.8] log of peak X-ray luminosity, in erg/s units</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_logEx</name><description>Limit flag on logEx</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logEx</name><description>[34.1/37.6] log of flare energy, in erg units</description><unit>log(1e-07J)</unit><ucd>em.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sf</name><description>Display this super-flare data (link to Table 4)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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>Name</name><description>Flare host star name (HHMMSS.ss+DDMMSS.s; J2000) (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column></table><table><name>J/ApJ/916/32/table4</name><description>Super-flares from protostellar candidates</description><column><name>Class</name><description>Flare Class (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>[52.2/344.1] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-47.6/75.2] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>alpha</name><description>[0.3/2.1]? IRAC SED slope, {alpha}</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Nphot</name><description>[21/296] Flare X-ray counts</description><unit>ct</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ME</name><description>[5/5.7] Flare median photon energy</description><unit>keV</unit><ucd>phys.energy;stat.median;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_logLxpk</name><description>Limit flag on logLxpk</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logLxpk</name><description>[31.3/33.8] log of peak X-ray luminosity, in erg/s units</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_logEx</name><description>Limit flag on logEx</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logEx</name><description>[34.9/37.6] log of flare energy, in erg units</description><unit>log(1e-07J)</unit><ucd>em.energy</ucd><dataType xsi:type="vs:VOTableType">float</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>Region</name><description>Star forming region (See Table 1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Name</name><description>X-ray host star name (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>ObsID</name><description>[1/6] X-ray Chandra observation as in Table 3 (G1)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>