Limits on the spatial variations of the electron-to-proton mass ratio in the Galactic plane

Free Access

Table 1

Source positions and radial velocities.

No.	Core	Position		V _LSR	Other name	Telescope
		α ₂₀₀₀	δ ₂₀₀₀	(km s^-1)		used
		(^h: ^m: ^s)	(°: ′: ′′)

1	L1498	04:10:51	+25:09:58	7.81		32-m/100-m
2	L1498A	04:10:58	+25:09:15	7.75		100-m
3	Do279P6	18:29:07	+00:30:51	7.75	Ser G3-G6 ^a	100-m
4	Do279P12	18:29:47	+01:14:53	7.59	BDN 31.57+5.37 ^b	100-m
5	SS3	18:29:57	−02:00:10	7.39		100-m
6	Do279P8	18:30:04	−02:48:14	8.52		100-m
7	Ka05	19:37:01	+07:34:30	8.40	B335^c, CB199^d	100-m
8	L1251C	22:35:54	+75:18:55	−4.73		100-m
9	L1512	05:04:10	+32:43:09	7.11		32-m/100-m

Reference. (a) Cohen & Kuhi (1979); (b) Dobashi et al. (2005); (c) Barnard (1927); (d) Clemens and Barvainis (1988).

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.