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<ri:Resource created="2021-08-06T13:25:48Z" 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>V346 Nor IJHKs photometry &amp; IR spectra</title><shortName>J/ApJ/889/148</shortName><identifier>ivo://CDS.VizieR/J/ApJ/889/148</identifier><altIdentifier>doi:10.26093/cds/vizier.18890148</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kospal A.</name></creator><creator><name>Szabo Z.M.</name></creator><creator><name>Abraham P.</name></creator><creator><name>Kraus S.</name></creator><creator><name>Takami M.</name></creator><creator><name>Lucas P.W.,Contreras Pena C.</name></creator><creator><name>Udalski A.</name></creator><date role="Updated">2022-01-17T11:51:03Z</date><date role="Created">2021-08-06T13:25:48Z</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>variable-stars</subject><subject>infrared-photometry</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>FU Orionis-type objects (FUors) are young low-mass stars undergoing powerful accretion outbursts. The increased accretion is often accompanied by collimated jets and energetic, large-scale molecular outflows. The extra heating during the outburst may also induce detectable geometrical, chemical, and mineralogical changes in the circumstellar material, affecting possible planet formation around these objects. V346 Nor is a southern FUor with peculiar spectral characteristics. Decades after the beginning of its outburst, it unexpectedly underwent a fading event around 2010 due to a decrease in the mass accretion rate onto the star by at least two orders of magnitude. Here we present optical and near-infrared photometry and spectroscopy obtained after the minimum. Our light curves show a gradual re-brightening of V346 Nor, with its Ks-band brightness only 1.5mag below the outburst brightness level. Our Very Large Telescope (VLT)/XSHOOTER spectroscopic observations display several strong forbidden emission lines toward the source from various metals and molecular hydrogen, suggesting the launch of a new jet. Our N-band spectrum obtained with VLT/VISIR outlines a deeper silicate absorption feature than before, indicating that the geometry of the circumstellar medium has changed in the post-outburst period compared to peak brightness.</description><source format="bibcode">2020ApJ...889..148K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/889/148</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/B/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/eso">B/eso : ESO Science Archive Catalog (ESO, 1991-2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/337">II/337 : VISTA Variables in the Via Lactea Survey DR1 (Saito+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/125/149">J/A+AS/125/149 : CHIANTI- An Atomic Database For Emission Lines I. 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Uncertainty on the Imag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</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>Date</name><description>Date of observation (UT)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>JD</name><description>[6438.27/8734.06] Julian Date; JD-2450000.5</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_Imag</name><description>Limit flag on Imag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Imag</name><description>[17.94/20.94]? I band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Jmag</name><description>[14.03/15.17]? J-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Jmag</name><description>[0.01/0.05]? Uncertainty on the Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Hmag</name><description>[11.41/12.87]? H-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Hmag</name><description>[0.01/0.02]? Uncertainty on the Hmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ksmag</name><description>[8.47/10.79]? Ks-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ksmag</name><description>[0.01/0.13]? Uncertainty on the Ksmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Inst</name><description>Instrument</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>n_Inst</name><description>[a] a=From Kospal+ 2017A&amp;A...597L..10K</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/ApJ/889/148/fig4</name><description>Average VLT/XSHOOTER spectrum of V346 Nor observed in 2015 June-July</description><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>Arm</name><description>VLT/XSHOOTER arm identifier (1)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>lambda</name><description>[0.3/2.48] Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[-1.93e-13/1.86e-13] Flux density; in erg/s/cm^2^/{AA} units</description><unit>cW.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/889/148/fig5</name><description>VLT/VISIR N-band spectrum of V346 Nor, obtained in the post-outburst phase on 2016 February 29</description><column><name>lambda</name><description>[6.7/14] Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</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>Flux</name><description>[-1866/37] Flux density</description><unit>Jy</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>