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<ri:Resource created="2025-11-12T15:18:08Z" status="active" updated="2025-11-12T14:34:55Z" 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>SPYGLASS. III. Fornax-Hor assoc. &amp; Austral complex</title><shortName>J/ApJ/941/143</shortName><identifier>ivo://CDS.VizieR/J/ApJ/941/143</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kerr R.</name></creator><creator><name>Kraus A.L.</name></creator><creator><name>Murphy S.J.</name></creator><creator><name>Krolikowski D.M.</name></creator><creator><name>Bedding T.R.,Rizzuto A.C.</name></creator><date role="Updated">2025-11-12T14:34:55Z</date><date role="Created">2025-11-12T15:18:08Z</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>stellar-associations</subject><subject>radial-velocity</subject><subject>line-intensities</subject><subject>stellar-masses</subject><subject>young-stellar-objects</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>two-color-diagrams</subject><description>The study of young associations is essential for building a complete record of local star formation processes. The Fornax-Horologium association (FH), including the {chi}1 Fornacis cluster, represents one of the nearest young stellar populations to the Sun. This association has recently been linked to the Tuc-Hor, Carina, and Columba associations, building an extensive "Austral Complex" almost entirely within 150pc. Using Gaia astrometry and photometry in addition to new spectroscopic observations, we perform the deepest survey of FH to date, identifying over 300 candidate members, nearly doubling the known population. By combining this sample with literature surveys of the other constituent populations, we produce a contiguous stellar population covering the entire Austral Complex, allowing the definitions of subpopulations to be reassessed along with connections to external populations. This analysis recovers new definitions for FH, Tuc-Hor, Columba, and Carina, while also revealing a connection between the Austral complex and the Sco-Cen-affiliated Platais 8 cluster. This suggests that the Austral complex may be just a small component of a much larger and more diverse star formation event. Computing ages and tracing stellar populations back to formation reveals two distinct nodes of cospatial and continuous formation in the Austral Complex, one containing Tuc-Hor, and the other containing FH, Carina, and Columba. This mirrors recent work showing similar structure elsewhere, suggesting that these nodes, which only emerge through the use of traceback, may represent the clearest discrete unit of local star formation, and a key building block needed to reconstruct larger star-forming events.</description><source format="bibcode">2022ApJ...941..143K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/941/143</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/B/ocl">B/ocl : Optically visible open clusters and Candidates (Dias+ 2002-2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/254">III/254 : 2nd Cat. of RVel with Astrometric Data (Kharchenko+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/137">V/137 : Extended Hipparcos Compilation (XHIP) (Anderson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/279">III/279 : RAVE 5th data release (Kunder+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/135/503">J/A+AS/135/503 : HIP southern B8-F2 stars radial velocities (Grenier+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/3356">J/AJ/123/3356 : Palomar/MSU nearby star sp. survey. 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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>Sp</name><description>spectroscopic properties (Table 1)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Gaia</name><description>Gaia DR3 source identifier</description><ucd>meta.id;meta.main</ucd><flag>primary</flag></column><column><name>Group</name><description>Literature group the star was initially assigned to (1)</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Src</name><description>Source the star was drawn from (2)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Reg</name><description>[1/6] ID of the HDBSCAN subgroup (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RA_ICRS</name><description>Right Ascension (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>plx</name><description>[3.5/20] Gaia DR3 parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><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>Gmag</name><description>[-0.2/5]? Gaia DR3 G-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GBP-GRP</name><description>[5.9/63] Gaia DR3 GBP-GRP color</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mstar</name><description>[0.09/3.7] Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>D</name><description>[0/1] Clustering proximity</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A</name><description>[0/1] Boolean solution to the Astrometric quality cut from SPYGLASS-I (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>P</name><description>[0/1] Boolean solution to the Photometric quality cut from SPYGLASS-I (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PY</name><description>[0/1] Flag for the photometric youth determination of the star (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>V</name><description>[-1/1] Flag to represent the results of our velocity membership cuts (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>F</name><description>[0/10]? Flag for other notable features (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/941/143/table1</name><description>Spectroscopic properties of members in Fornax- Horologium and the connected Tuc-Hor, Columba, and Carina associations</description><column><name>Gaia</name><description>Gaia DR3 source identifier</description><ucd>meta.id;meta.main</ucd></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>RA_ICRS</name><description>Right Ascension (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>RVel</name><description>[-26/94]? Radial Velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_RVel</name><description>[0/37.4]? Uncertainty in RVel</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_RVel</name><description>Source for RVel (see refs.dat file)</description><ucd>meta.ref;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>EWLi</name><description>[-0.09/2.3]? Equivalent width, Lithium</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_EWLi</name><description>[0/1.9]? Uncertainty in EWLi</description><unit>0.1nm</unit><ucd>stat.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_EWLi</name><description>Source for EWLi (see refs.dat file)</description><ucd>meta.ref;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>EWHb</name><description>[-36.8/3.8]? Equivalent width, H{beta}</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>e_EWHb</name><description>[0/1]? Uncertainty in EWHb</description><unit>0.1nm</unit><ucd>stat.error;spect.line.eqWidth;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_EWHb</name><description>Source for EWHb (see refs.dat file)</description><ucd>meta.ref;spect.line.eqWidth;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table><table><name>J/ApJ/941/143/table5</name><description>Binaries in the Austral complex (see Section 3.3)</description><column><name>Gmag</name><description>[4.6/19.7] Gaia DR3 G-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>[6.6/34.3] Gaia DR3 parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><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>Gaia</name><description>Gaia DR3 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>Syst</name><description>[0/100] Sequential system identifier</description><ucd>meta.id;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>m_Syst</name><description>Number of stars in this system</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Sep</name><description>[0/8533] Projected separation (1)</description><unit>au</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RA_ICRS</name><description>Right Ascension (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/941/143/refs</name><description>References</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>Ref</name><description>Reference code</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Auth</name><description>First author's name(s)</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>BibCode</name><description>Bibcode of the reference</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Comm</name><description>Comment</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="59*">char</dataType></column></table></schema></tableset></ri:Resource>