The local group symbiotic star population and its tenuous link with type Ia supernovae

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Table 1.

Coordinates, distances, proper motions, and radial velocities of the analyzed stars.

ID	Name	RA	Dec	r	δr	PM_RA	δPM_RA	PM_Dec	δPM_Dec	RV	δRV	RV Ref.	IR type
		[°]	[°]	[pc]		[mas yr⁻¹]		[mas yr⁻¹]		[km s⁻¹]
1	EG And	11.15500	40.67929	590	20	8.61	0.03	−15.47	0.02	−95.0	0.16	(1)	S
2	AX Per	24.09457	54.25064	2100	300	−1.82	0.02	−5.86	0.03	−117.4	0.1	(2)	S
3	V471 Per	29.70694	52.89679	2500	200	0.46	0.02	−2.29	0.02	−30	20	(3)	D’
4	BD Cam	55.53868	63.21689	230	30	−17.88	0.23	20.05	0.30	−22.3	0.1	(4)	S
5	StHA 32	69.44015	−1.31999	10 000	3000	5.2	0.02	−4.21	0.02	322	1	(5)	S
6	V1261 Ori	80.57690	−8.66614	370	30	47.14	0.11	−4.172	0.097	79.77	0.09	(6)	S
...	...	...	...	...	...	...	...	...	...	...	...	...	...

Notes. The entire table is available in electronic form at the CDS. Column 1 gives the SySt ID in our sample, while column 2 gives its assigned name as in the New Online Database of Symbiotic Variables Merc et al. (2019a,b), referred also to the catalog of Akras et al. (2019). Columns 3 and 4 display observed right ascension and declination in degrees. Columns 5 and 6 give the geometric distance as in Bailer-Jones et al. (2021) and its uncertainty. Right ascension and declination proper motions, as well as their uncertainties, in Gaia DR3 are displayed in columns 7 to 10. Radial velocity, its uncertainty, and reference are displayed in columns 11, 12, and 13, respectively. Column 14 provides the IR class of the SySt (S-, D-, or D’-type) as in Akras et al. (2019), Merc et al. (2019a,b). Displayed RVs and distance uncertainty values are raised according to the systematic uncertainty analysis described in Section 3.1. Distance and RV values are rounded according to their respective uncertainties. (1) Fekel et al. (2000b); (2) Fekel et al. (2000a); (3) Gaia DR3 (Gaia Collaboration 2023); (4) Griffin (1984); (5) Pereira et al. (2017); (6) Boffin et al. (2014); (7) Dumm et al. (1998); (8) Carquillat & Prieur (2008); (9) Fekel et al. (2017); (10) Jorissen et al. (2019); (11) Reimers et al. (1988); (12) Kenyon & Garcia (1989); (13) Gałan et al. (2022); (14) Fekel et al. (2015); (15) Schild et al. (1996); (16) Smith et al. (1997); (17) Fekel et al. (2007); (18) Ferrer et al. (2003); (19) Hinkle et al. (2019); (20) Fekel et al. (2008); (21) Hinkle et al. (2006); (22) Munari et al. (2021); (23) Munari et al. (1994); (24) Fekel et al. (2010); (25) Brandi et al. (2009); (26) Fekel et al. (2001); (27) Brandi et al. (2003); (28) Hinkle et al. (2009); (29) Brandi et al. (2006); (30) Harries & Howarth (2000); (31) Gromadzki & Mikołajewska (2009).

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