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Table 7.

Association of pulsator in the all sky sample with open/globular clusters and with dwarf galaxies satellites of the MW.

Source_id Lit. name Classification Host system Source of association
(1) (2) (3) (4) (5)
428620663657823232 DL Cas DCEP_F NGC129 A13
429385923752386944 CG Cas DCEP_F Berkeley58 A13
2011892320749270912 CE Cas B DCEP_F NGC7790 A13
2011892325047232256 CE Cas A DCEP_F NGC7790 A13
2011892703004353792 CF Cas DCEP_F NGC7790 A13
2031776202613700480 SU Cyg DCEP_F Turner9 A13
4085919765884068736 BB Sgr DCEP_F Collinder394 A13
4092905375639902464 U Sgr DCEP_F IC4725 A13
4094784475310672128 WZ Sgr DCEP_F Turner2 A13
4156512638614879104 EV Sct DCEP_1O NGC6664 A13
5835124087174043136 S Nor DCEP_F NGC6087 A13
5891675303053080704 V Cen DCEP_F NGC5662 A13
5932565900081831040 QZ Nor DCEP_1O NGC6067 A13
5932569709575669504 V340 Nor DCEP_F NGC6067 A13
2957940098405233024 V7 WVIR NGC1904 C01

Notes. The different columns correspond to the following: (1) Gaia DR2 source identification; (2) name of the object in the literature (if any); (3) type of variability according to this work; (4) host system; (5) source of the association of the variable with the stellar system. The table is published in its entirety only at the CDS. A portion including the first 15 lines is shown for guidance regarding its form and content.

References. A13 (Anderson et al. 2013); B05 (Bersier & Wood 2002); C01 (Clement et al. 2001); CO15 (Coppola et al. 2015); DR1 (Clementini et al. 2016); EROS2_KIM (Kim et al. 2014); K08 (Kinemuchi et al. 2008); MV16 (Martínez-Vázquez et al. 2016); OGLE (Optical Gravitational Lensing Experiment, Soszyński et al. 2015a,b, 2016, 2017a,b, 2018); TW (This work).

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