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Table 2
Limits used for the Gaia data query and results from the kinematic members selection.
ID | RA | Dec | ϖ | μα | μδ |
---|---|---|---|---|---|
(J2000) | (J2000) | (mas) | (mas yr−1) | (mas yr−1) | |
Query range | 07h13m to 07h15m | −12°35′ to −11°45′ | 0.4 to 2 | −7 to 1 | −4 to 4 |
P ≥ 50% | 07h13.m7 to 07h14.m4 | −12°14′ to −11°58′ | 0.87 ± 0.30 | −3.26 ± 0.44 | 1.08 ± 0.46 |
CMa06 | 07h03.m7 to 07h05.m6 | −11°34′ to −11°00′ | 0.85 ± 0.09 | −4.18 ± 0.36 | 1.52 ± 0.21 |
Sh 2-296 | 07h01.m2 to 07h06.m8 | −12°12′ to −10°48′ | 0.8 to 1.25 | −4.10 ± 0.60 | 1.50 ± 0.40 |
Notes. Our sample (P ≥ 50%) is compared with clusters CMa06 (Santos-Silva et al. 2021) and Sh 2-296 (Gregorio-Hetem et al. 2021) located to the W direction of the CMa shell.
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