Comparing the spatial and kinematic distribution of gas and young stars around the shell-like structure in the CMa OB1 association

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Table A.1

Membership probability, parallax, proper motion, and Gaia EDR3 photometry.

Gaia EDR3	P	ϖ	μ_α	μ_δ	G	G_BP	G_RP
	%	mas	mas/yr	mas/yr	mag	mag	mag
3045239083971370112	87	0.77 ± 0.17	− 3.21 ± 0.16	0.91 ± 0.15	18.65	20.43	17.24
3045208886056506112	13	1.69 ± 1.10	− 2.52 ± 0.86	0.97 ± 1.06	20.33	21.63	18.78

3045225516172964864^a	95	0.66 ± 0.02	− 3.32 ± 0.02	0.74 ± 0.02	13.80	14.77	12.74
3045229291445342592^b	92	1.31 ± 0.19	− 3.26 ± 0.18	0.98 ± 0.16	18.80	20.42	17.43
3045227749555916032^c	91	0.61 ± 0.14	− 3.11 ± 0.16	0.88 ± 0.13	17.93	19.59	16.63
3045131301773079168	90	0.79 ± 0.10	− 3.02 ± 0.08	1.04 ± 0.09	17.44	19.06	16.22
3045208950479742208	83	1.12 ± 0.26	− 3.28 ± 0.20	1.11 ± 0.18	18.89	20.72	17.57
3045237434703416320	82	1.63 ± 0.39	− 3.52 ± 0.34	1.09 ± 0.33	19.89	21.26	18.52
3045235785435946624	79	0.72 ± 0.32	− 3.13 ± 0.26	1.22 ± 0.24	19.03	20.96	17.65
3045117141257872000	78	1.00 ± 0.30	− 3.49 ± 0.28	0.90 ± 0.29	19.01	20.52	17.75
3045215998525392384^d	65	0.97 ± 0.11	− 2.93 ± 0.11	0.43 ± 0.10	17.29	19.13	15.91
3045116114758900736	65	0.57 ± 0.52	− 4.38 ± 0.53	1.48 ± 0.54	19.99	21.22	18.57
3045114804796665984	63	1.02 ± 0.51	− 3.17 ± 0.44	2.00 ± 0.48	19.85	21.54	18.39
3045214070080777600	27	0.92 ± 1.18	− 2.78 ± 0.90	0.44 ± 1.00	20.66	21.37	19.22
3045234170527254656	21	0.45 ± 0.10	− 3.00 ± 0.10	0.87 ± 0.09	17.39	19.19	16.07
3045235785436006400	21	1.47 ± 0.80	− 3.48 ± 0.62	0.54 ± 0.63	20.26	21.51	18.81

3045118416872687744	92	0.96 ± 0.03	− 3.69 ± 0.03	0.99 ± 0.03	12.85	12.97	12.63
3045226821842999552	97	0.80 ± 0.05	− 3.51 ± 0.06	1.03 ± 0.06	16.32	17.39	15.29
3045213352825581312	97	0.89 ± 0.02	− 3.28 ± 0.02	0.99 ± 0.02	14.03	14.49	13.40
3045228368031224448	96	0.84 ± 0.05	− 3.23 ± 0.05	1.15 ± 0.05	15.86	16.64	14.99
3045215758007221632	94	0.79 ± 0.04	− 3.19 ± 0.04	0.94 ± 0.04	15.85	16.76	14.87
3045232555619709056	93	1.17 ± 0.02	− 3.60 ± 0.02	0.83 ± 0.02	14.50	14.87	13.97
3045114809098665984	92	0.76 ± 0.02	− 3.22 ± 0.01	1.01 ± 0.01	12.60	12.99	12.02
3045229291444432384	90	0.50 ± 0.18	− 4.08 ± 0.16	1.06 ± 0.14	18.59	20.14	17.32
3045114701716408832	90	0.90 ± 0.21	− 3.53 ± 0.18	1.11 ± 0.20	18.70	20.30	17.46
3045114843459884288	90	0.87 ± 0.41	− 3.71 ± 0.33	1.46 ± 0.36	19.60	20.97	18.36
3045209156636885760	85	0.72 ± 0.13	− 2.71 ± 0.11	0.94 ± 0.09	17.68	19.11	16.52
3045114396781820672	84	0.91 ± 0.03	− 3.11 ± 0.02	0.96 ± 0.02	14.53	14.88	14.02
3045118382511875712	82	0.88 ± 0.05	− 3.90 ± 0.04	0.97 ± 0.04	15.81	16.43	15.05
3045227509039371648	80	0.44 ± 0.37	− 2.95 ± 0.36	0.94 ± 0.30	19.39	20.99	18.11
3045233242814458752	79	0.67 ± 0.19	− 2.92 ± 0.20	1.19 ± 0.22	18.63	20.13	17.47
3045229879859736704	70	0.51 ± 0.10	− 4.33 ± 0.09	1.11 ± 0.10	17.53	18.91	16.38
3045207885326442496	70	1.27 ± 0.31	− 3.06 ± 0.24	0.87 ± 0.23	19.34	20.71	18.19
3045228952146750208	70	0.55 ± 0.13	− 2.88 ± 0.14	1.02 ± 0.12	18.11	20.01	16.81
3045130678995758848	69	1.37 ± 0.28	− 3.63 ± 0.33	1.67 ± 0.34	19.26	20.84	17.97
3045130472837058176	66	1.56 ± 0.59	− 2.26 ± 0.70	0.83 ± 0.72	20.20	21.74	18.88
3045420954362862336	64	1.38 ± 0.03	− 3.52 ± 0.03	1.56 ± 0.03	15.32	15.85	14.62
3045212936208209024	64	0.60 ± 0.39	− 2.34 ± 0.30	1.02 ± 0.33	19.33	20.77	18.11
3045233693790633472	62	1.25 ± 0.19	− 2.80 ± 0.17	1.70 ± 0.16	18.58	19.99	17.43
3045233281473783936	59	0.92 ± 0.01	− 3.01 ± 0.02	1.00 ± 0.02	13.50	13.92	12.89
3045213623404184448	58	1.37 ± 0.40	− 2.63 ± 0.36	0.66 ± 0.31	19.46	21.21	18.14
3045233998728534272	56	0.56 ± 0.37	− 2.45 ± 0.29	1.47 ± 0.27	19.58	20.97	18.31
3045233487625692160	53	0.81 ± 0.57	− 3.79 ± 0.78	1.65 ± 0.95	20.07	21.24	18.75
3045225202636012800	50	1.06 ± 0.58	− 3.88 ± 0.61	0.45 ± 0.64	20.04	21.43	18.73

Notes: The objects are distinguished by: Class I (top); Class II (middle); Class III (bottom), according with Table A.2. Stars identified as Hα emitters are indicated by (a) ID 381; (b) ID 387; (c) ID 390; and (d) ID 392, where the ID numbers are given by Pettersson & Reipurth (2014).

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