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<ri:Resource created="2022-01-07T08:57:14Z" 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>Infrared spectra of V838 Monocerotis with SOFIA</title><shortName>J/AJ/162/183</shortName><identifier>ivo://CDS.VizieR/J/AJ/162/183</identifier><altIdentifier>doi:10.26093/cds/vizier.51620183</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Woodward C.E.</name></creator><creator><name>Evans A.</name></creator><creator><name>Banerjee D.P.K.</name></creator><creator><name>Liimets T.</name></creator><creator><name>Djupvik A.A.,Starrfield S.</name></creator><creator><name>Clayton G.C.</name></creator><creator><name>Eyres S.P.S.</name></creator><creator><name>Gehrz R.D.</name></creator><creator><name>Wagner R.M.</name></creator><date role="Updated">2022-03-14T06:37:38Z</date><date role="Created">2022-01-07T08:57:14Z</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>multiple-stars</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>Luminous Red Variables are most likely eruptions that are the outcome of stellar mergers. V838Mon is one of the best-studied members of this class, representing an archetype for stellar mergers resulting from B-type stars. As result of the merger event, "nova-like" eruptions occur driving mass loss from the system. As the gas cools considerable circumstellar dust is formed. V838Mon erupted in 2002 and is undergoing very dynamic changes in its dust composition, geometry, and infrared luminosity providing a real-time laboratory to validate mineralogical condensation sequences in stellar mergers and evolutionary scenarios. We discuss recent NASA Stratospheric Observatory for Infrared Astronomy 5-38{mu}m observations combined with archival NASA Spitzer spectra that document the temporal evolution of the freshly formed (within the last &lt;~20yr) circumstellar material in the environs of V838Mon. Changes in the 10{mu}m spectral region are strong evidence that we are witnessing a classical dust condensation sequence expected to occur in oxygen-rich environments where alumina formation is followed by that of silicates at the temperature cools.</description><source format="bibcode">2021AJ....162..183W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/162/183</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/J/A+AS/146/437">J/A+AS/146/437 : IR spectra of oxygen-rich evolved stars (Speck+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/28/764">J/PAZh/28/764 : UBVR photometry of Nova Mon 2002 (V838 Mon) (Goranskii+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/598/L43">J/ApJ/598/L43 : Polarimetry of V838 Mon and stars around (Wisniewski+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/434/1107">J/A+A/434/1107 : UBVRIc photometry of stars around V838 Mon (Munari+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/84/147">J/AZh/84/147 : Light curves of V838 Mon and V4332 Sgr (Goranskii+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/532/A138">J/A+A/532/A138 : V838 Mon spectrum in 2009 (Tylenda+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/553/A81">J/A+A/553/A81 : Refraction of corundum, spinel, {alpha}-quartz (Zeidler+,2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/630/A75">J/A+A/630/A75 : Six luminous red novae photometry (Pastorello+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/638/A17">J/A+A/638/A17 : VLBA SiO masers toward V838 Monocerotis (Ortiz-Leon+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/646/A119">J/A+A/646/A119 : M31 luminous red nova AT 2019zhd photometry (Pastorello+,2021)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/162/183</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/162/183</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/162/183</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/162/183</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/162/183</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/162/183</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/162/183/fig1</name><description>V838 Mon SOFIA FORCAST spectra</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>Wave</name><description>[5.1/36.9] Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[5.34/38] Flux density</description><unit>Jy</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>[0.07/3] Uncertainty in Flux</description><unit>Jy</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>