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<ri:Resource created="2016-05-04T07:14:00Z" 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>Atmosphere parameters model-derived for PMS &amp; BDs</title><shortName>J/ApJ/805/57</shortName><identifier>ivo://CDS.VizieR/J/ApJ/805/57</identifier><altIdentifier>doi:10.26093/cds/vizier.18050057</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tottle J.</name></creator><creator><name>Mohanty S.</name></creator><date role="Updated">2017-12-15T10:55:37Z</date><date role="Created">2016-05-04T07:14:00Z</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>stellar-spectral-types</subject><subject>effective-temperature</subject><subject>extinction</subject><subject>young-stellar-objects</subject><subject>astronomical-models</subject><subject>infrared-photometry</subject><description>We test state-of-the-art model atmospheres for young very-low-mass stars and brown dwarfs in the infrared, by comparing the predicted synthetic photometry over 1.2-24{mu}m to the observed photometry of M-type spectral templates in star-forming regions. We find that (1) in both early and late young M types, the model atmospheres imply effective temperatures (Teff) several hundred Kelvin lower than predicted by the standard pre-main sequence (PMS) spectral type-Teff conversion scale (based on theoretical evolutionary models). It is only in the mid-M types that the two temperature estimates agree. (2) The Teff discrepancy in the early M types (corresponding to stellar masses &gt;~0.4M_{sun}_ at ages of a few Myr) probably arises from remaining uncertainties in the treatment of atmospheric convection within the atmospheric models, whereas in the late M types it is likely due to an underestimation of dust opacity. (3) The empirical and model-atmosphere J-band bolometric corrections are both roughly flat, and similar to each other, over the M-type Teff range. Thus the model atmospheres yield reasonably accurate bolometric luminosities (Lbol), but lead to underestimations of mass and age relative to evolutionary expectations (especially in the late M types) due to lower Teff. We demonstrate this for a large sample of young Cha I and Taurus sources. (4) The trends in the atmospheric model J-K_s_ colors, and their deviations from the data, are similar at PMS and main sequence ages, suggesting that the model dust opacity errors we postulate here for young ages also apply at field ages.</description><source format="bibcode">2015ApJ...805...57T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/805/57</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/95">J/ApJ/767/95 : Improved parameters of smallest KIC stars (Dressing+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/8">J/ApJ/731/8 : Multiple star formation in Taurus-Auriga (Kraus+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/196/4">J/ApJS/196/4 : New young star candidates in Taurus-Auriga (Rebull+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/259">J/ApJS/186/259 : Taurus Spitzer survey: new candidate members (Rebull+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/111">J/ApJS/186/111 : Spitzer observations of Taurus members (Luhman+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/684/654">J/ApJ/684/654 : Low-mass members of Chamaeleon I (Luhman+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/675/1375">J/ApJ/675/1375 : IRAC/MIPS photometry in Cha I (Luhman+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/478/507">J/A+A/478/507 : Distances &amp; 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