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<ri:Resource created="2024-01-23T12:20:12Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Follow-up monitoring of Gaia20eae</title><shortName>J/ApJ/927/125</shortName><identifier>ivo://CDS.VizieR/J/ApJ/927/125</identifier><altIdentifier>doi:10.26093/cds/vizier.19270125</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cruz-Saenz de Miera F.</name></creator><creator><name>Kospal A.</name></creator><creator><name>Abraham P.</name></creator><creator><name>Park S.</name></creator><creator><name>Nagy Z.</name></creator><creator><name>Siwak M.,Kun M.</name></creator><creator><name>Fiorellino E.</name></creator><creator><name>Szabo Z.M.</name></creator><creator><name>Antoniucci S.</name></creator><creator><name>Giannini T.</name></creator><creator><name>Nisini B.,Szabados L.</name></creator><creator><name>Kriskovics L.</name></creator><creator><name>Ordasi A.</name></creator><creator><name>Szakats R.</name></creator><creator><name>Vida K.</name></creator><creator><name>Vinko J.,Zielinski P.</name></creator><creator><name>Wyrzykowski L.</name></creator><creator><name>Garcia-Alvarez D.</name></creator><creator><name>Drozdz M.</name></creator><creator><name>Ogloza W.,Sonbas E.</name></creator><date role="Updated">2024-11-06T20:23:39Z</date><date role="Created">2024-01-23T12:20:12Z</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>young-stellar-objects</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We present follow-up photometric and spectroscopic observations, and subsequent analysis of Gaia20eae. This source triggered photometric alerts during 2020 after showing a ~3mag increase in its brightness. Its Gaia Alert light curve showed the shape of a typical eruptive young star. We carried out observations to confirm Gaia20eae as an eruptive young star and classify it. Its pre-outburst spectral energy distribution shows that Gaia20eae is a moderately embedded Class II object with L_bol_=7.22L_{sun}_. The color-color and color-magnitude diagrams indicate that the evolution in the light curve is mostly gray. Multiple epochs of the H{alpha} line profile suggest an evolution of the accretion rate and winds. The near-infrared spectra display several emission lines, a feature typical of EX Lupi-type (EXor) eruptive young stars. We estimated the mass accretion rate during the dimming phase to be dM/dt=3-8x10^-7^M_{sun}_/yr, higher than typical T Tauri stars of similar mass and comparable to other EXors. We conclude Gaia20eae is a new EXor-type candidate.</description><source format="bibcode">2022ApJ...927..125C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/927/125</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>related-to</relationshipType><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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2413">J/AJ/136/2413 : Galactic midplane Spitzer red sources (Robitaille+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/321">J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/18">J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/192">J/AJ/144/192 : Spitzer survey of Orion A and B. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>JD</name><description>Julian date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Filt</name><description>Broadband filter (gri or BVRcIc)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>omag</name><description>[13.48/22.5] Observed magnitude in Filt</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_omag</name><description>[0.0036/0.2] Uncertainty in omag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tel</name><description>Telescope used ("RC80", "Adiyaman" or "Suhora")</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column></table></schema></tableset></ri:Resource>