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<ri:Resource created="2023-08-24T08:44:44Z" 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>Near infrared view on PDRs</title><shortName>J/other/AstBu/78</shortName><identifier>ivo://CDS.VizieR/J/other/AstBu/78.373</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kirsanova M.S.</name></creator><creator><name>Tatarnikov A.M.</name></creator><creator><name>Boley P.A.</name></creator><creator><name>Vibe D.A.</name></creator><creator><name>Maclennikova N.A.,Tatarnikov A.A.</name></creator><date role="Updated">2025-01-09T07:52:04Z</date><date role="Created">2023-08-24T08:44:44Z</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>galaxies</subject><subject>infrared-sources</subject><subject>h-ii-regions</subject><subject>interstellar-medium</subject><subject>chemical-abundances</subject><description>We performed photometric observations of the S255, S257, S140, NGC7358 and the Orion Bar photo-dissociation regions (PDRs) at 2 micron using narrow-band filters centered on the Br-gamma, H2 and [FeII] lines, as well as the narrow-band Kcont and the broad-band H filters for continuum subtraction. The observations were done with the 2.5-m telescope of the SAI Caucasian Mountain Observatory and the near-infrared camera and spectrograph ASTRONIRCAM. We find several high-density arc-like structures in the Br-gamma and [FeII] images of the ionized gas in NGC 7538 and extended shells and arcs visible through the H2 emission. The H ionization front and H2 dissociation front are merged in NGC 7538. In S 255 and S 257 we detected only Br-gamma emission from the H II regions and bright H2 emission from the PDRs. The projected distance between the H ionization and H2 dissociation fronts are approx. 0.3-0.4pc, which cannot be explained using models of a uniform medium. Most probably, the ionized and neutral gas in these PDRs is clumpy. The H I-to-H2 transitions in the NGC 7538, S 255, S 257 and S 140 PDRs are gradual with no sharp borders. 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