J/A+A/463/589ivo://CDS.VizieR/J/A+A/463/589doi:10.26093/cds/vizier.34630589CDSSzekely P.Kiss L.L.Jackson R.Derekas A.Csak B.Szatmary K.2007-06-17T08:03:14Z2007-06-17T08:00:52ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frglobular-star-clustersvariable-starsradial-velocityccd-photometryNGC 362 is a bright southern globular cluster in the foreground of the Small Magellanic Cloud (SMC), for which no extensive variability survey has ever been done. Finding regularly pulsating RR Lyrae stars in the cluster can lead to improved metallicity and distance estimates of the system, while other types of variable objects may be used to confirm the results. Time-series CCD photometric observations have been obtained. Light curves have been derived with both profile fitting photometry and image subtraction. We developed a simple method to convert flux phase curves to magnitudes, which allows the use of empirical light curve shape vs. physical parameters calibrations. Periods and light curve parameters of the detected variable stars have been determined with Fourier analysis, phase dispersion minimization and string-length minimization. Using the RR Lyrae metallicity and luminosity calibrations, we have determined the relative iron abundances and absolute magnitudes of the stars. The color-magnitude diagram has been fitted with Yale-Yonsei isochrones to determine reddening and distance independently. For five RR Lyrae stars we obtained radial velocity measurements from optical spectra. We found 45 RR Lyr stars, of which the majority are new discoveries. While most of them are cluster members, as shown by their radial velocities and positions in the color-magnitude diagram, we also see a few stars in the galactic field and in the outskirts of the SMC. About half of the RR Lyraes exhibit light curve changes (Blazhko effect). The RR Lyrae-based metallicity of the cluster is [Fe/H]=-1.16+/-0.25, the mean absolute magnitude of the RR Lyrae stars is M_V=0.82+/-0.04mag implying a distance of 7.9+/-0.6kpc. The mean period of RRab stars is 0.585+/-0.081days. These properties place NGC 362 among the Oosterhoff type I globular clusters. The isochrone fit implies a slightly larger distance of 9.2+/-0.5kpc and an age of 11+/-1Gyr. We also found 11 eclipsing binaries, 14 pulsating stars of other types, including classical Cepheids in the SMC and 15 variable stars with no firm classification. NGC 362 hosts a large number of RR Lyrae stars, which makes the cluster a potentially important test object for studying the Blazhko effect in a chemically homogeneous environment.2007A&A...463..589Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/463/589CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+AS/93/311 : Relative proper motions in NGC 362 (Tucholke 1992)J/AJ/106/1508 : Dynamics of globular cluster NGC 362 (Fischer+ 1993)J/AJ/122/2569 : VI photometry of NGC 288, 362 and 1851 (Bellazzini+, 2001)J/MNRAS/351/1204 : IR Photometry of 10 Galactic Globular Clust. (Valenti+ 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/463/589https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/463/589http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/463/589https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/463/589https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/463/589http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/463/589GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/463/589/varstars (Variables coordinates)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/463/589/varstars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/463/589/varstars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/463/589/varstars?GETtext/xml+votable180.050000true15.23602917-71.028838890.005555555555555556Cone search capability for table J/A+A/463/589/stars (Celestial coordinates and standard V and V-I of NGC 362 stars (only the central CCD segment))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/463/589/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/463/589/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/463/589/stars?GETtext/xml+votable180.050000true16.26222083-70.949669440.0055555555555555566/33330https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/463/589?format=asciiOpticaldefaultJ/A+A/463/589/varstarsVariables coordinatesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintVNameVariable numbermeta.id;meta.maincharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainisisName of file in isis subdirectory (Flux vs HJD)meta.id;meta.filecharpsfName of file in psf subdirectory (dmag vs HJD)meta.id;meta.filecharrvName of file in rv subdirectory (RV vs HJD)meta.id;meta.filecharrvpName of file in rvp subdirectory (RV vs phase)meta.id;meta.filecharJ/A+A/463/589/starsCelestial coordinates and standard V and V-I of NGC 362 stars (only the central CCD segment)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainxposx coordinatepixpos.cartesian.x;instr.detdoubleyposy coordinatepixpos.cartesian.y;instr.detdoubleVmagstandard V magnitudemagphot.mag;em.opt.VfloatV-Istandard V-I magnitudemagphot.color;em.opt.V;em.opt.Ifloat