M37 variable stars

DOI

We have conducted a deep (15~<r~<23 ), 20 night survey for transiting planets in the intermediate-age (~550Myr) open cluster M37 (NGC 2099) using the Megacam wide-field mosaic CCD camera on the 6.5m MMT. In this paper we present a catalog and light curves for 1445 variable stars; 1430 (99%) of these are new discoveries. We have discovered 20 new eclipsing binaries and 31 new short-period (P~500) that are members of the cluster. We identify and analyze five particularly interesting individual variables, including a previously identified variable that we suggest is probably a hybrid gamma Doradus/delta Scuti pulsator, two possible quiescent cataclysmic variables, a detached eclipsing binary (DEB) with at least one gamma Doradus pulsating component (only the second such variable found in an eclipsing binary), and a low-mass (M_P_~M_S~0.6M_{sun} DEB that is a possible cluster member. A preliminary determination of the physical parameters for the DEB+gamma Doradus system yields M_P=1.58+/-0.04M_{sun}, M_S=1.58+/-0.04M_{sun}, R_P=1.39+/-0.07R_{sun}, and R_S=1.38+/-0.07R_{sun}_.

Cone search capability for table J/ApJ/675/1254/m37var (Variables and suspected variables in M37)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16751254
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/675/1254
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/675/1254
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/675/1254
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/675/1254
Provenance
Creator Hartman J.D.; Gaudi B.S.; Holman M.J.; McLeod B.A.; Stanek K.Z.,Barranco J.A.; Pinsonneault M.H.; Kalirai J.S.
Publisher CDS
Publication Year 2010
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Physics; Stellar Astronomy