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<ri:Resource created="2013-09-25T07:43:01Z" 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>YSOs in LDN 1641 with Hectochelle spectra</title><shortName>J/ApJS/207/5</shortName><identifier>ivo://CDS.VizieR/J/ApJS/207/5</identifier><altIdentifier>doi:10.26093/cds/vizier.22070005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fang M.</name></creator><creator><name>Kim J.S.</name></creator><creator><name>van Boekel R.</name></creator><creator><name>Sicilia-Aguilar A.</name></creator><creator><name>Henning T.,Flaherty K.</name></creator><date role="Updated">2017-07-03T14:25:58Z</date><date role="Created">2013-09-25T07:43:01Z</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>accretion</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>infrared-photometry</subject><subject>young-stellar-objects</subject><subject>line-intensities</subject><subject>stellar-spectral-types</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><description>We investigate the young stellar objects (YSOs) in the Lynds 1641 (L1641) cloud using multi-wavelength data including Spitzer, WISE, the Two Micron All Sky Survey, and XMM covering ~1390 YSOs across a range of evolutionary stages. In addition, we targeted a sub-sample of YSOs for optical spectroscopy with the MMT/Hectospec and the MMT/Hectochelle. We use these data, along with archival photometric data, to derive spectral types, extinction values, masses, ages, and accretion rates. We obtain a disk fraction of ~50% in L1641. The disk frequency is almost constant as a function of stellar mass with a slight peak at log (M_*_/M_{sun}_){approx}-0.25. The analysis of multi-epoch spectroscopic data indicates that the accretion variability of YSOs cannot explain the two orders of magnitude of scatter for YSOs with similar masses. Forty-six new transition disk (TD) objects are confirmed in this work, and we find that the fraction of accreting TDs is lower than for optically thick disks (40%-45% versus 77%-79%, respectively). We confirm our previous result that the accreting TDs have a median accretion rate similar to normal optically thick disks. We confirm that two star formation modes (isolated versus clustered) exist in L1641. We find that the diskless YSOs are statistically older than the YSOs with optically thick disks and the TD objects have a median age that is intermediate between those of the other two populations. We tentatively study the star formation history in L1641 based on the age distribution and find that star formation started to be active 2-3 Myr ago.</description><source format="bibcode">2013ApJS..207....5F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/207/5</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/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><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/746/154">J/ApJ/746/154 : Sco-Cen members spectroscopy (Pecaut+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A109">J/A+A/533/A109 : Pisa pre-main sequence tracks and isochrones (Tognelli+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/504/461">J/A+A/504/461 : Paper I. 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H{alpha} equivalent width; in units of Angstroms</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHa.1</name><description>[27/612]? H{alpha} full width at 10% peak intensity</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>TTS</name><description>[C/W] T Tauri type (C=classical or W=weak)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Prob</name><description>[0/100]? Accretor probability</description><unit>%</unit><ucd>stat</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_logMac</name><description>Limit flag on logMac</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logMac</name><description>[-12.2/-7]? Log of mass 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>Date</name><description>Date of the observation</description><ucd>time.epoch</ucd><flag>nullable</flag></column></table><table><name>J/ApJS/207/5/prop</name><description>Stellar and disk properties, masses and ages of the YSOs, in L1641</description><column><name>Age1</name><description>[0/66]? Age from D08 (1)</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Disk</name><description>Disk type (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>l_logMHb</name><description>Limit flag on logMHb</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><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>Seq</name><description>[1/1388] Running sequence number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SpT</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>L</name><description>[0.005/448.72] Luminosity</description><unit>solLum</unit><ucd>phys.luminosity;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Av</name><description>[0/9.8] The V band extinction</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EWHa</name><description>[-407/2.6]? H{alpha} equivalent width in {AA}</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHb</name><description>[-87/69]? H{beta} equivalent width in {AA}</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_logMHa</name><description>Limit flag on logMHa</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logMHa</name><description>[-12/-5]? Log mass accretion rate from H{alpha}</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>logMHb</name><description>? Log mass accretion rate from H{beta}</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>TTS</name><description>[C/W] T Tauri star type (C=Classical, or W=Weak)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>M1</name><description>[0.1/4.5]? Mass from D08 (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_M1</name><description>[0/0.83]? Lower limit uncertainty in M1</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_M1</name><description>[0/0.63]? Upper limit uncertainty in M1</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Age1</name><description>[0/49.6]? Lower limit uncertainty in Age1</description><unit>Myr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Age1</name><description>[0/36.9]? Upper limit uncertainty in Age1</description><unit>Myr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M2</name><description>[0.1/3.7]? Mass from S00 (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_M2</name><description>? Lower limit uncertainty in M2</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_M2</name><description>? Upper limit uncertainty in M2</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age2</name><description>[0.1/72]? Age from S00 (1)</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Age2</name><description>? Lower limit uncertainty in Age2</description><unit>Myr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Age2</name><description>? Upper limit uncertainty in Age2</description><unit>Myr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M3</name><description>[0.05/1.4]? Mass from B98 (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_M3</name><description>? Lower limit uncertainty in M3</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_M3</name><description>? Upper limit uncertainty in M3</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age3</name><description>[1/43.1]? Age from B98 (1)</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Age3</name><description>? Lower limit uncertainty in Age3</description><unit>Myr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Age3</name><description>? Upper limit uncertainty in Age3</description><unit>Myr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M4</name><description>[0.06/2.9]? Mass from DM97 (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_M4</name><description>? Lower limit uncertainty in M4</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_M4</name><description>? Upper limit uncertainty in M4</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age4</name><description>[0/74.8]? Age from DM97 (1)</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Age4</name><description>? Lower limit uncertainty in Age4</description><unit>Myr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Age4</name><description>? Upper limit uncertainty in Age4</description><unit>Myr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M5</name><description>[0.2/4.7]? Mass from Pisa11 (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_M5</name><description>? Lower limit uncertainty in M5</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_M5</name><description>? Upper limit uncertainty in M5</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age5</name><description>[0.2/56.1]? Age from Pisa11 (1)</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Age5</name><description>? Lower limit uncertainty in Age5</description><unit>Myr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Age5</name><description>? Upper limit uncertainty in Age5</description><unit>Myr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>