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<ri:Resource created="2012-07-03T12:45:33Z" 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>Formaldehyde maser flares in IRAS 18566+0408</title><shortName>J/ApJ/717/L133</shortName><identifier>ivo://CDS.VizieR/J/ApJ/717/L133</identifier><altIdentifier>doi:10.26093/cds/vizier.17179133</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Araya E.D.</name></creator><creator><name>Hofner P.</name></creator><creator><name>Goss W.M.</name></creator><creator><name>Kurtz S.</name></creator><creator><name>Richards A.M.S.</name></creator><creator><name>Linz H.,Olmi L.</name></creator><creator><name>Sewilo M.</name></creator><date role="Updated">2012-07-20T20:21:43Z</date><date role="Created">2012-07-03T12:45:33Z</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>young-stellar-objects</subject><subject>interstellar-masers</subject><subject>radio-astronomy</subject><subject>interstellar-medium</subject><description>We report results of an extensive observational campaign of the 6cm formaldehyde maser in the young massive stellar object IRAS 18566+0408 (G37.55+0.20) conducted from 2002 to 2009. Using the Arecibo Telescope, the Very Large Array, and the Green Bank Telescope, we discovered quasi-periodic formaldehyde flares (P~237 days). Based on Arecibo observations, we also discovered correlated variability between formaldehyde (H_2_CO) and methanol (CH_3_OH) masers. The H_2_CO and CH_3_OH masers are not spatially coincident, as demonstrated by different line velocities and high angular resolution MERLIN observations. The flares could be caused by variations in the infrared radiation field, possibly modulated by periodic accretion onto a young binary system.</description><source format="bibcode">2010ApJ...717L.133A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/717/L133</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/VI/51">VI/51 : Collisional Excitation Rates of Formaldehyde (Green 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/391/869">J/MNRAS/391/869 : A mapping survey of massive CO cores (Guan+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/669/435">J/ApJ/669/435 : Arecibo Methanol Maser Galactic Plane Survey. II. (Pandian+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/432/737">J/A+A/432/737 : General Catalogue of 6.7GHz Methanol Masers (Pestalozzi+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/845">J/A+A/368/845 : Arcetri Catalog of H2O maser sources. Update. (Valdettaro+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/276/57">J/MNRAS/276/57 : IRAS Galactic star-forming regions. II. 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