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<ri:Resource created="2023-09-12T06:10:42Z" status="active" updated="2026-07-02T11:44:21Z" 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>Spectroscopic study of Ba and CEMP-s stars</title><shortName>J/AJ/165/154</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/154</identifier><altIdentifier>doi:10.26093/cds/vizier/be-55-4t</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Goswami P.P.</name></creator><creator><name>Goswami A.</name></creator><date role="Updated">2026-07-02T11:44:21Z</date><date role="Created">2023-09-12T06:10:42Z</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>a-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><subject>effective-temperature</subject><description>We have performed detailed high-resolution spectroscopic analysis on seven metal-poor stars (BD+75348, BD+093019, HD238020, HE0319-0215, HE0507-1653, HE0930-0018, HE1023-1504) and derived their atmospheric parameters Teff, logg, [Fe/H], and microturbulent velocity ({xi}). The metallicity range is found to be -2.57&lt;[Fe/H]&lt;-0.42. The elemental abundances of 17 light elements and 12 heavy elements are estimated. We have classified BD+75348 and BD+093019 as strong Ba stars, HD238020 as a mild Ba star, and the remaining four objects as CEMP-s stars. We have estimated the masses of the stars from Hertzsprung-Russel (HR) diagram, and, compiling the data of 205 Ba stars from literature, estimated the mass distribution of Ba stars. We have also estimated the initial masses of the companion AGBs of the program stars as well as the masses of the companion AGBs of 159 Ba and 36 CEMP-s stars from literature, with the help of a parametric-model-based analysis using FRUITY models. While the primary mass distribution of mild Ba stars peaks at 3.7M{sun}, for the strong Ba stars the peak appears at 2.5M{sun}. We, therefore, propose that the initial masses of the progenitor AGBs dominantly control the formation of mild and strong Ba stars. However, a clear overlap, in the range 1.3-4.0M{sun}, noticed between the progenitor masses of both the subclasses of Ba stars, may indicate that other factors, such as the metallicities and the orbital periods, may also have significant contributions. The progenitor AGBs' mass distribution of CEMP-s stars is found to peak at 2.03M{sun}.</description><source format="bibcode">2023AJ....165..154G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/154</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</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/V/81">V/81 : Taxonomy of Barium Stars (Lu 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/275/101">J/A+A/275/101 : Chemical evolution of galactic disk I. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>RAJ2000</name><description>[3/15] 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>Ref</name><description>Spectrum reference(s)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Bmag</name><description>[9.34/16.3] B-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>[8.49/14.7] V-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag</name><description>[6.9/12.4] J-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>[6.51/11.7] H-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>[6.38/11.5] K-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Texp</name><description>[1200/2700] Exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Obs</name><description>Observation date, day</description><ucd>time.epoch;obs</ucd></column><column><name>S/N4000</name><description>[7/70] Signal-to-Noise ratio at 4000{AA}</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S/N6000</name><description>[25/200] Signal-to-Noise ratio at 6000{AA}</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RVel</name><description>[-258/350] Radial velocity estimates in this work</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[0.3/4] Error on RVel</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVel-G</name><description>[-233/354]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ion</name><description>Element identifier FeI or FeII</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Wave</name><description>[4187/6740] Wavelength in Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Elow</name><description>[0/4.99] Lower excitation energy</description><unit>eV</unit><ucd>phys.atmol.excitation;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf</name><description>[-4.95/0.52] log oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BD+75348</name><description>[42.2/188.2]? Equivalent width in BD+75-348</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[BD+75348]</name><description>[6.74/7.48]? Derived abundance in BD+75-348</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BD+093019</name><description>[32.7/197]? Equivalent width in BD+09-3019</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[BD+093019]</name><description>[6.58/7.23]? Derived abundance in BD+09-3019</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HD238020</name><description>[20.7/222]? Equivalent width in HD238020</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HD238020]</name><description>[6.51/7.22]? Derived abundance in HD238020</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE03190215</name><description>[35.5/1233]? Equivalent width in HE0319-0215</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE03190215]</name><description>[4.76/5.16]? Derived abundance in HE0319-0215</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE05081653</name><description>[29.3/180]? Equivalent width in HE0508-1653</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE05081653]</name><description>[5.83/6.22]? Derived abundance in HE0508-1653</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE09300018</name><description>[20.2/153]? Equivalent width in HE 0930-0018</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE09300018]</name><description>[5.93/6.3]? Derived abundance in HE0930-0018</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE10231504</name><description>[29.4/164]? Equivalent width in HE 1023-1504</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE10231504]</name><description>[5.61/6.08]? Derived abundance in HE1023-1504</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/AJ/165/154/table6</name><description>Equivalent widths of Fe-lines used for the calculation of elemental abundances</description><column><name>loggf</name><description>[-5.7/0.69] log oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BD+75348</name><description>[23.0/191.2]? Equivalent width in BD+75 348</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[BD+75348]</name><description>[1.49/7.59]? Derived abundance in BD+75-348</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BD+093019</name><description>[69.7/180]? Equivalent width in BD+093019</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[BD+093019]</name><description>[2.43/8.31]? Derived abundance in BD+093019</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></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>Wave</name><description>[4061/6768] Wavelength in Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ion</name><description>Element identifier</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Elow</name><description>[0/5.61] Lower excitation energy</description><unit>eV</unit><ucd>phys.atmol.excitation;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HD238020</name><description>[8.1/339]? Equivalent width in HD238020</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HD238020]</name><description>[0.36/7.38]? Derived abundance in HD238020</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE03190215</name><description>[21.9/119]? Equivalent width in HE0319-0215</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE03190215]</name><description>[0.01/5.51]? Derived abundance in HE03190215</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE05081653</name><description>[14.3/149]? Equivalent width in HE0508-1653</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE05081653]</name><description>[1.25/6.81]? Derived abundance in HE0508-1653</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE09300018</name><description>[18.5/180]? Equivalent width in HE0930-0018</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE09300018]</name><description>[0.35/6.69]? Derived abundance in HE09300018</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HE10231504</name><description>[29.7/162]? Equivalent width in HE1023-1504</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[HE10231504]</name><description>[1.14/5.67]? Derived abundance in HE1023-1504</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/AJ/165/154/table13</name><description>Masses of the Ba-stars and initial masses of their AGB companions</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">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>Name</name><description>Star identifier (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Teff</name><description>[3609/6440] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[0.6/4.6] log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-1.11/0.23] Metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[ls/Fe]</name><description>[-0.14/1.75]? log average abundance of light-s process elements</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[hs/Fe]</name><description>[0.17/2.13] log average abundance of heavy-s process elements</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[hs/ls]</name><description>[-0.37/0.98]? log abundance difference of heavy-s to light-s process elements</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mass</name><description>[0.8/4.5]? Ba star mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Massi</name><description>[1.5/6]? Initial stellar AGB mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>chi2</name><description>[0.01/43.2]? Model {chi}^2^ value</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dil</name><description>[0.0009/1.91]? Dilution factor</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Nel</name><description>[4/16]? Number of elements used in analysis</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Type</name><description>Type of Ba stars</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ref</name><description>Reference code (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>_RA</name><description>Position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>_DE</name><description>Position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column></table><table><name>J/AJ/165/154/table14</name><description>Initial masses of AGB companions of CEMP-s stars</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>_DE</name><description>Position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></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>Name</name><description>Star identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Teff</name><description>[4000/6625] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[0.5/4.3] log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-3/-1.29] Metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Massi</name><description>[1.3/3]? Initial stellar AGB mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>chi2</name><description>[0.19/24.8] Model {chi}^2^ value</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dil</name><description>[0.001/1.76] Dilution factor</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Nel</name><description>[4/12] Number of elements used in analysis</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>