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<ri:Resource created="2020-09-23T08:32:19Z" 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>Post-AGB candidates in LMC and SMC SALT spectra</title><shortName>J/A+A/641/A142</shortName><identifier>ivo://CDS.VizieR/J/A+A/641/A142</identifier><altIdentifier>doi:10.26093/cds/vizier.36410142</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Szczerba R.</name></creator><creator><name>Hajduk M.</name></creator><creator><name>Pavlenko</name></creator><creator><name>Ya.V.</name></creator><creator><name>Hrivnak B.J.</name></creator><creator><name>Kaminsky</name></creator><creator><name>B.M.,Volk K.</name></creator><creator><name>Siodmiak N. Gezer I.</name></creator><creator><name>Zacs L.</name></creator><creator><name>Pych W.</name></creator><creator><name>Sarna M.</name></creator><date role="Updated">2021-09-08T06:42:03Z</date><date role="Created">2020-09-23T08:32:19Z</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>magellanic-clouds</subject><subject>giant-stars</subject><subject>spectroscopy</subject><description>We selected a sample of post-AGB candidates in the Magellanic Clouds on the basis of their near- and mid-infrared colour characteristics. Fifteen of the most optically bright post-AGB candidates were observed with the South African Large Telescope in order to determine their stellar parameters and thus to validate or discriminate their nature as post-AGB objects in the Magellanic Clouds. The spectral types of absorption-line objects were estimated according to the MK classification, and effective temperatures were obtained by means of stellar atmosphere modelling. Emission-line objects were classified on the basis of the fluxes of the emission lines and the presence of the continuum. Out of 15 observed objects, only 4 appear to be genuine post-AGB stars (27%). In the SMC, 1 out of 4 is post-AGB, and in the LMC, 3 out 11 are post-AGB objects. Thus, we can conclude that the selected region in the colour-colour diagram, while selecting the genuine post-AGB objects, overlaps severely with other types of objects, in particular young stellar objects and planetary nebulae. Additional classification criteria are required to distinguish between post-AGB stars and other types of objects. In particular, photometry at far-IR wavelengths would greatly assist in distinguishing young stellar objects from evolved ones. 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