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<ri:Resource created="2020-04-01T06:50:54Z" 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>Fried Egg Nebula AMBER and GRAVITY observations</title><shortName>J/A+A/635/A183</shortName><identifier>ivo://CDS.VizieR/J/A+A/635/A183</identifier><altIdentifier>doi:10.26093/cds/vizier.36350183</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Koumpia E.</name></creator><creator><name>Oudmaijer R.D.</name></creator><creator><name>Graham V.</name></creator><creator><name>Banyard G.</name></creator><creator><name>Black J.H.,Wichittanakom C.</name></creator><creator><name>Ababakr K.M.</name></creator><creator><name>de Wit W.-J.</name></creator><creator><name>Millour F.</name></creator><creator><name>Lagadec E.,Muller S.</name></creator><creator><name>Cox N.L.J.</name></creator><creator><name>Zijlstra A.</name></creator><creator><name>van Winckel H.</name></creator><creator><name>Hillen M.</name></creator><creator><name>Szczerba R.,Vink J.S.</name></creator><creator><name>Wallstrom S.H.J.</name></creator><date role="Updated">2020-08-21T08:22:50Z</date><date role="Created">2020-04-01T06:50:54Z</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>giant-stars</subject><subject>interferometry</subject><subject>spectroscopy</subject><description>The objective of this work is to study in detail the nature (i.e., geometry, rates) of the mass-loss episodes associated with the yellow hypergiant IRAS 17163-3907. We analysed a large set of optical/near-infrared data, in spectroscopic, photometric, spectropolarimetric, and interferometric modes. We use the optical observations to determine its spectral type and we present the first model independent reconstructed images of IRAS 17163-3907 at 2 micron tracing milli-arcsecond scales. 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