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<ri:Resource created="2024-09-27T12:03:55Z" status="active" updated="2026-03-20T00:00:00Z" 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>YSOs in GRSMC 045.49+00.04 from IR obs.</title><shortName>J/other/PASA/41.</shortName><identifier>ivo://CDS.VizieR/J/other/PASA/41.55</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Azatyan N.</name></creator><creator><name>Nikoghosyan E.</name></creator><creator><name>Samsonyan A.</name></creator><creator><name>Elia D.</name></creator><creator><name>Kaper L.</name></creator><creator><name>Yeghikyan A.,Andreasyan D.</name></creator><creator><name>Baghdasaryan D.</name></creator><date role="Updated">2025-02-13T07:48:56Z</date><date role="Created">2024-09-27T12:03:55Z</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>molecular-clouds</subject><subject>h-ii-regions</subject><subject>young-stellar-objects</subject><subject>infrared-photometry</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><subject>extinction</subject><subject>interstellar-medium</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>stellar-distance</subject><description>Understanding the characteristics of young stellar populations is essential for deriving insights into star formation processes within parent molecular clouds and the influence of massive stars on these processes. This study primarily aims to investigate the young stellar objects (YSOs) within the molecular cloud G 045.49+00.04, including three ultra-compact HII (UC HII) regions: G 45.48+0.13 (IRAS19117+1107), G 45.45+0.06 (IRAS 19120+1103), and G 45.47+0.05. We used near-, mid-, and far-infrared photometric data along with radiation transfer models and the modified blackbody fitting to identify and study the YSOs and the interstellar medium (ISM). In total, we identified 1482 YSOs in a 12 arcmin radius covering GRSMC 045.49+00.04, with a mass range from 1.5M_{sun}_ to 22M_{sun}_. Of these, 315 objects form relatively dense clusters in the UC HII regions, close to the IRAS 19120+1103 and 19117+1107 sources. In each UC HII region, several high-mass stars have been identified, which in all likelihood are responsible for the ionization. The YSOs with 21.8M_{sun}_ and 13.7+/-0.4M_{sun}_ are associated with IRAS 19120+1103 and 19117+1107, respectively. The non-cluster YSOs (1168) are uniformly distributed on the field. The distribution of YSOs from both samples on the colour-magnitude diagram and by the evolutionary ages is different. About 75% of objects in the IRAS clusters are concentrated around the Zero Age Main Sequence and have a well-defined peak at an age of Log(Age[years])~6.75, with a narrow spread. The non-cluster objects have two concentrations located to the right and left of the 0.1Myr isochrone and two well-defined peaks at Log(Age)~6.25 and 5.25. The fraction of the near-infrared excess stars, as well as the mass function confirm that the evolutionary age of the cluster is about 1Myr. The K luminosity functions' {alpha} slopes for the IRAS clusters and non-cluster objects are 0.32+/-0.04 and 0.72+/-0.13, respectively. The steeper {alpha} slope is suggesting that the non-cluster objects are less evolved, which is well consistent with the evolutionary age. Similar results -- including evolutionary age, narrow age spread, and the less evolved nature of non-cluster objects -- were also observed for the YSOs in the neighbouring G 45.14+00.14. The both regions (G045.49+00.04 and G45.14+00.14) are located and distinguished by their brightness and density at the edge of the bubble around the highly variable X-ray binary GRS 1915+105, which includes a black hole and a K-giant companion. Based on the above, we can assume that the process of star formation in the young IRAS clusters was triggered by the GRS 1915+105-initiated shock front inside the ISM massive condensation, through the process of "collecting and collapse". Most non-cluster objects probably belong to a later generation. Their formation could be triggered by the recurrent activity of GRS 1915+105 and/or through the edge collapse scenario and mass accumulation through the gas flows along the ISM filaments.</description><source format="bibcode">2024PASA...41...55A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/PASA/41.55</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/125">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/293">II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/316">II/316 : UKIDSS-DR6 Galactic Plane Survey (Lucas+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/139">VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/106">VIII/106 : Herschel/PACS Point Source Catalogs (Herschel team, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/64">J/AJ/149/64 : MIPSGAL 24{mu}m point source catalog (Gutermuth+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/591/A149">J/A+A/591/A149 : Hi-GAL. 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IRAS 25um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F25</name><description>[0/32000]? rms uncertainty on F25</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F60</name><description>[0/5340000]? IRAS 60um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F60</name><description>[0/373800]? rms uncertainty on F60</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F100</name><description>[0/7890000]? IRAS 100um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F100</name><description>[0/3945000]? rms uncertainty on F100</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F70</name><description>[0/127275]? Herschel PACS 70um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F70</name><description>[0/525]? rms uncertainty on P_F70</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F160</name><description>[0/160355]? Herschel PACS 160um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F70Hi</name><description>[0/1552000]? HiGAL 70um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F70Hi</name><description>[0/1600]? rms uncertainty on H_F70</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F160Hi</name><description>[0/842000]? HiGAL 160um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F160Hi</name><description>[0/1900]? rms uncertainty on F160</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F250</name><description>[0/465000]? HiGAL 250um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F250</name><description>[0/1859]? rms uncertainty on F250</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F350</name><description>[0/178498]? HiGAL 350um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F350</name><description>[0/1814]? rms uncertainty on F350</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F500</name><description>[0/96000]? HiGAL 500um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.400-750GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F500</name><description>[0/3141]? rms uncertainty on F500</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.mm.400-750GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Region</name><description>Region</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>F12</name><description>[0/78800]? IRAS 12um measured flux</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_F160</name><description>[0/156339]? rms uncertainty on P_F160</description><unit>mJy</unit><ucd>stat.error;phot.mag;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/other/PASA/41.55/table3</name><description>Parameters of IRAS sources derived from Robitaille+ 2007ApJS..169..328R models SED fitting</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>UKIDSS hour of right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>UKIDSS degree of declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Nd</name><description>[3/12] Number of input fluxes</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Av</name><description>[5/54.4] Interstellar extinction</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Av</name><description>[0/11.5] Av rms uncertainty</description><unit>mag</unit><ucd>stat.error;phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[5.99/9] Distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dist</name><description>[0/4.1] Dist rms uncertainty</description><unit>kpc</unit><ucd>stat.error;pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logAge</name><description>[3.17/6.91] Log of stellar age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logAge</name><description>[0/6.6] logAge rms uncertainty</description><unit>log(yr)</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[1.5/21.8] Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>[0/6.7] Mass rms uncertainty</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Temp</name><description>[4119/30328] Temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Temp</name><description>[0/10003] Temp rms uncertainty</description><unit>K</unit><ucd>stat.error;phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMd</name><description>[-7.84/-0.27]? log of disk mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logMd</name><description>[-9.01/0]? logMd rms uncertainty</description><unit>log(solMass)</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MdotE</name><description>[-10.4/4.6]? Envelope accretion rate</description><unit>log(solMass.yr**-1)</unit><ucd>phys.mass.loss</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MdotD</name><description>[-13.4/-3.95]? Disk accretion rate</description><unit>log(solMass.yr**-1)</unit><ucd>phys.mass.loss</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MdotD</name><description>[-16.2/0]? MdotD rms uncertainty</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error;phys.mass.loss</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LumTot</name><description>[1.38/5] log of total luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_LumTot</name><description>[0/4.3] LumTot rms uncertainty</description><unit>log(solLum)</unit><ucd>stat.error;phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Region</name><description>Region</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>ID</name><description>[9/1482] ID number in final list of members</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_MdotE</name><description>[-10.64/0]? MdotE rms uncertainty</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error;phys.mass.loss</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>IRAS</name><description>IRAS name (IHHMMm+DDMM; B1950)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Nfit</name><description>[1/999] Number of fitted models</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>