New stellar bow shocks and bubbles found around runaway stars

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Table 1

Data of the 10 out of 106 GOSC-Gaia DR3 runaway stars with higher values of E in decreasing order.

Runaway id	GOSC name	Gaia DR3 id	RA	Dec	d	$μ_{α, corr}^{}$ $\mu _{\alpha ,{\rm{corr}}}^ $	µ_δ,corr	G	S.T.	$V_{PEC}^{2 D}$ $V_{{\rm{PEC}}}^{2{\rm{D}}}$	E	Run. Ref.	Bow. Ref.
			(h m s)	(°′ ″)	(kpc)	(mas yr⁻¹)	(mas yr⁻¹)			(km s⁻¹)
GR1	V479 Sct	4104196427943626624	18 26 15.06	−14 50 54.4	1.94	7.178	−6.866	10.80	ON6	90.9 ± 4.9	4.28	1	–
GR2	CPD −34 2135	5546501254035205376	08 13 35.36	−34 28 43.9	3.23	5.848	−2.894	9.18	O7.5	85.1 ± 5.6	3.85	2	–
GR3	BD +60 134	427457895747434880	00 56 14.21	61 45 36.9	2.69	2.928	−5.840	10.40	O5.5	77.9 ± 4.8	3.70	3	–
GR4	HD 104 565	6072058878595295488	12 02 27.77	−58 14 34.3	4.72	−8.694	4.853	9.07	OC9.7	193.7 ± 25.2	3.47	2	–
GR5	HD 155 913	5953699131931631232	17 16 26.32	−42 40 04.0	1.21	−9.539	7.676	8.18	O4.5	70.6 ± 4.5	3.43	2	–
GR6	HD 75 222	5625488726258364544	08 47 25.13	−36 45 02.5	2.09	0.123	6.320	7.31	O9.7	67.4 ± 6.9	3.03	2	–
GR7	ALS 12 688	2003815312630659584	22 55 44.94	56 28 36.6	4.34	4.061	−1.815	10.39	O5.5	74.5 ± 6.8	2.90	3	–
GR8	BD −14 5040	4104201586232296960	18 25 38.91	−14 45 05.8	1.63	5.548	−3.423	10.02	O5.5	50.4 ± 2.3	2.87	2	I, II
GR9	HD 41 997	3345950879898371712	06 08 55.82	1542 18.0	1.75	-0.586	−9.374	8.30	O7.5	77.3 ± 9.1	2.79	2	–
GR10	Y Cyg	1869256701670871168	20 52 03.58	34 39 27.2	1.39	4.731	−11.691	7.26	O9.5	82.1 ± 10.0	2.78	2	–

Notes. Run. Ref. (Runaway Reference) column provides a reference in case the star had already been reported as runaway: (1) Ribó et al. (2002); (2) Maíz Apellániz et al. (2018); (3) Kobulnicky & Chick (2022). Bow. Ref. (Bowshock Reference) column provides a reference in case the star had already been reported as having a bow shock: (I) Peri et al. (2015); (II) Kobulnicky et al. (2016). The proper motions corrected for the ISM motion caused by Galactic rotation (see text) are $μ_{α, corr}^{*}$ $\mu _{\alpha ,{\rm{corr}}}^ *$ and μ_δ,corr (with $μ_{α, corr}^{*} = μ_{α, corr} \cos δ$ $\mu _{\alpha ,{\rm{corr}}}^ * = {\mu _{\alpha ,{\rm{corr}}}}\cos \delta$ ). The complete version of this table including the 106 classified runaways is available at the CDS.

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