MWSC clustersivo://org.gavo.dc/mwsc/q/cluThe GAVO DC teamKharchenko, N.V.Piskunov, A.E.Roeser, S.Schilbach, E.Scholz, R.-D.2021-07-20T07:25:57ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837surveysopen-star-clustersstellar-kinematicsgalaxy-structureproper-motions MWSC presents a list of 3006 Milky Way Stellar Clusters (MWSC), found in the 2MAst (2MASS with Astrometry) catalogue. The target list was compiled on the basis of present-day lists of open, globular and candidate clusters. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, mean cluster proper motions, distances, reddenings, ages, tidal parameters, and sometimes radial velocities.2013A&A...558A..53Khttp://dc.g-vo.org/mwsc/q/clu/infoIsServedByGAVO Data Center TAP servicehttp://dc.g-vo.org/MWSChttps://dc.g-vo.org/MWSChttp://dc.g-vo.org/mwsc/q/clu/scs.xml?https://dc.g-vo.org/mwsc/q/clu/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealrecnoMWSC sequential number (cluster catalog number).meta.id;meta.maincharot_certainTrue if the object type is confirmed, false if object type has candidate status.meta.code;src.classcharnameNGC, IC or other common designationmeta.idcharobject_typeObject typesrc.classcharrclusterAngular radius of the clusterdegphys.angSize;srcrealdistDistance from the Sunpcpos.distance;pos.heliocentricreallogtLogarithm of average agelog(yr)time.age;stat.meanrealfe_hMetallicity [Fe/H]; this is copied from 2013arXiv1309.4325C or 2012A&A...539A.125D. Data for globular clusters is taken from the revised Harris (1996) catalogue, edition 2010, or newly determined.phys.abund.FerealresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integer180100000true0.067560.9330.001http://dc.g-vo.org/mwsc/q/clu/capabilitieshttps://dc.g-vo.org/mwsc/q/clu/capabilitieshttp://dc.g-vo.org/mwsc/q/clu/availabilityhttps://dc.g-vo.org/mwsc/q/clu/availabilityhttp://dc.g-vo.org/mwsc/q/clu/tableMetadatahttps://dc.g-vo.org/mwsc/q/clu/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tap2/86,165 3/17,19-20,22,25,28,46-47,49-51,56-58,202,207,218-219,221-223,225,228-229,240-241,244-245,325,327,333,336,338-339,369-370,374,377,380-382,448,450-451,454,456-457,460,472,478-479,581,583,589,591-594,600,606,613,615,620-621,623,626-627,634,642,649-654,658-659,664,668,671-672 4/28,53,64,66-67,72-74,84,86,92,94,96-98,107,109,111,116-118,120-122,124,132,139,149,151-152,156,166,169,174-176,178,181-183,192-193,208,210-211,214,218,221-222,237-238,240,242,248,251-252,254,268,270,293,384,388,392,394-395,399,417-418,422,426,430,589,600,604,625,645-646,649,775-776,779,781,783,793,800,804,806-807,813-815,818,824,847,854,861-866,871,880-881,896-898,905-907,909-911,920-922,925-926,929,944-945,968,970,973-974,984,987-990,992,1008,1011-1013,1015,1030,1040,1070,1193,1230,1285-1286,1292,1296-1297,1299,1304,1306,1312-1313,1331,1339-1342,1349-1350,1360,1363,1369-1371,1394,1396,1398-1400,1402,1404,1406,1425,1428-1430,1437,1439,1461,1463,1473-1475,1484-1485,1487-1488,1490-1491,1494,1501-1503,1505,1507,1514-1516,1518-1519,1532-1534,1541,1552,1568,1571,1617,1748-1749,1754,1780,1796,1798,1808-1810,1814,1822-1823,1832-1833,1835-1837,1839,1844-1846,1849,1851-1853,1856,1858-1861,1863-1864,1866,1874,1882,1885,1893-1896,1898,1900-1902,1904,1906-1909,1911,1921,1923,1925-1926,1937-1938,1940-1941,1943-1945,1962-1963,1984-1986,1988,1991-1993,1996,1999,2005-2006,2008,2014,2029,2032,2038,2054,2066,2068,2070,2082-2083,2099,2102,2116,2131,2140-2141,2158,2200,2309-2310,2313,2317,2319-2320,2323,2329-2331,2342,2345,2349,2353-2355,2361,2363,2385,2387-2388,2390,2392,2394,2404,2406-2408,2410-2414,2418,2422,2436-2438,2445,2447-2449,2451,2456-2457,2459,2470,2472,2477-2479,2489-2491,2496-2498,2500-2502,2528,2530-2531,2534,2540,2543,2546,2553,2555,2563,2566,2574-2576,2578,2581,2583,2586-2587,2589-2591,2593-2595,2620,2623-2626,2628-2629,2661,2663,2665,2668-2670,2676-2678,2681,2692,2694-2696,2698-2699,2701,2704,2706,2708,2713-2714,2717,2720-2721,2723,2725-2726,2740,2753,2755,2763,2768,2772,2776,2825,2871,2944-2945,2948,2952,2956,2976,2979,2981-2982,2984,2986,2988-2989,2991,2993-2995,2997-2998,3000,3002-3003,3007,3020,3027,3043,3059http://dc.g-vo.org/mwsc/q/clu/coveragemwsc MWSC presents a list of 3006 Milky Way Stellar Clusters (MWSC), found in the 2MAst (2MASS with Astrometry) catalogue. The target list was compiled on the basis of present-day lists of open, globular and candidate clusters. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, mean cluster proper motions, distances, reddenings, ages, tidal parameters, and sometimes radial velocities.output MWSC presents a list of 3006 Milky Way Stellar Clusters (MWSC), found in the 2MAst (2MASS with Astrometry) catalogue. The target list was compiled on the basis of present-day lists of open, globular and candidate clusters. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, mean cluster proper motions, distances, reddenings, ages, tidal parameters, and sometimes radial velocities.membersLink to stars that are candiadate members of this clustermeta.ref.urlcharnullable_rDistance to cone centerdegpos.angDistancedoublenullablerecnoMWSC sequential number (cluster catalog number).meta.id;meta.maincharnameNGC, IC or other common designationmeta.idcharnullableconfirmation_flagIs this object a stellar cluster? 'dupe' indicates the object coincides with another cluster.charobject_typeObject typesrc.classcharnullablesourceSource for MWSC list and input parametersmeta.refcharnullablesource_typeObject type from sourcesrc.classcharnullablen_starNumber of stars in MWSC sky area.meta.number00.011195.054257.1799999999716431931.0intraj2000Adopted cluster centre in RA J2000.0degpos.eq.ra;meta.main0.067519.4204167.11343.301359.7720.794397doublenullabledej2000Adopted cluster centre in Dec J2000.0degpos.eq.dec;meta.main-83.445-64.7943-12.325563.774585.2550.794397doublenullableglonGalactic longitudedegpos.galactic.lon0.0088.31210.733351.439359.7640.794397doublenullableglatGalactic latitudedegpos.galactic.lat-89.386-18.2523-0.34616.457384.4930.794397doublenullablercoreAngular radius of the coredegphys.angSize;src0.0090.010.0180.050.50.794397floatnullablercenterAngular radius of the central partdegphys.angSize;src0.020.0350.070.249252.510.794397floatnullablerclusterAngular radius of the clusterdegphys.angSize;src0.040.0650.130.484256.20.794397floatnullablepmraAverage proper motion in RA*cos(DE)deg/yrpos.pm;pos.eq.ra;stat.mean-1.12361e-05-2.92736e-06-5.90278e-071.10833e-069.94444e-060.794397floatnullablepmdeAverage proper motion in Declinationdeg/yrpos.pm;pos.eq.dec;stat.mean-1.27778e-05-2.21625e-06-4.05556e-072.03111e-067.61111e-060.794397floatnullablee_pmError of proper motiondeg/yrstat.error;pos.pm;pos.eq.ra;stat.mean8.33333e-095.55556e-081.52778e-074.02778e-078.88889e-070.794397floatnullablervAverage radial velocitykm/sspect.dopplerVeloc;pos.heliocentric;stat.mean-411.4-123.815-4.57113.6474940.25185floatnullablee_rvError of RVkm/sstat.error;spect.dopplerVeloc;pos.heliocentric;stat.mean0.010.12.414.7138570.203488floatnullablen1s_coreNumber of most probable (1sigma) members within R(core)meta.number01.03.018.01470.7943975intnullablen1s_centerNumber of most probable (1sigma) members within R(center); these are the stars used to compute the average proper motion.meta.number28.030.0185.84999999999999500.7943975intnullablen1s_clusterNumber of most probable (1sigma) members within R(cluster)meta.number717.081.0513.042620.7943975intnullabledistDistance from the Sunpcpos.distance;pos.heliocentric87502.052069.58921.35825350.794397floatnullablecol_ex_optColour excess in (B-V)magphot.color.excess;phot.color;em.opt.B;em.opt.V00.0310.572.0823.7270.794397floatnullablelogtLogarithm of average agelog(yr)time.age;stat.mean66.28.6410.110.10.794397floatnullablercKing core radiuspcphys.size.radius0.080.31.246.62239.10.782505floatnullablertKing tidal radiuspcphys.size.radius0.843.0568.5836.212178.830.782505floatnullablekingkKing normalization factor (a measure of the central density of the cluster, see 2007A&A...468..151Ppc**-2stat.fit.param0.010.245.0950.8552384.030.781977floatnullablefe_hMetallicity [Fe/H]; this is copied from 2013arXiv1309.4325C or 2012A&A...539A.125D. Data for globular clusters is taken from the revised Harris (1996) catalogue, edition 2010, or newly determined.phys.abund.Fe-2.155-1.887-0.3340.2014290.1280.102273floatnullablenote_textThe text of the note for an object.meta.notecharnullable