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

Open Access

Table 2.

Inferred velocities of the analyzed star, together with the dynamical classification.

ID	Name	v_r	δv_r	v_φ	δv_φ	v_z	δv_z	Classification^a
		[km s⁻¹]		[km s⁻¹]		[km s⁻¹]
1	EG And	−38.7	0.1	133.4	0.2	2.1	0.2	TD
2	AX Per	−71.1	0.6	155.2	0.2	−36	1	TD
3	V471 Per	14	2	201	2	−13.1	0.5	D
4	BD Cam	−42.9	0.22	241.4	0.3	10.23	0.09	D
5	StHA 32	239.6	0.7	−125	9	−55	3	H
6	V1261 Ori	51.56	0.02	143.9	0.7	41.7	0.9	TD
...	...	...	...	...	...	...	...	...

Notes. The entire table is available in electronic form at the CDS. Columns 1 and 2 display the SySt ID in our sample and 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 to 8 provide the velocity components derived, and their respective uncertainties, namely: v_r radial velocity (in the galactic plane), v_φ azimuthal tangent velocity, v_z velocity perpendicular to the galactic plane. Column 9 provides the dynamic classification of the SySt (see in the main text ^aTD – thick disk, D – thin disk, H – halo, IB – “in-between”).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.