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Table 2

Results of the VLBA, LBA, and EVN observations.

Interferometer Transition Results for the brightest maser spot
RA (J2000) Dec (J2000) Vp Sp ΔVLSR
Day-of-the-year (GHz) (h m s) (° ′ ″) (km s−1) (Jy beam−1) (km s−1)
VLBA DOY: 270 6.7 CH3OH 18 35 08.14243±0.00007 −07 35 03.9242±0.0010 115.3 2.34 107.5–120.0
12.2 CH3OH 18 35 08.13433±0.00006 −07 35 04.2806±0.0008 110.3 0.97 110.1–112.1
22.2 H2O(a) 18 35 08.13231±0.00008 −07 35 04.1437±0.0012 125.1 7.72 122.1–127.1
VLBA DOY: 300 6.7 CH3OH 18 35 08.14235±0.00007 −07 35 03.9269±0.0010 115.4 5.80 107.5–120.1
12.2 CH3OH 18 35 08.13428±0.00006 −07 35 04.2815±0.0008 110.3 1.03 110.0–112.1
22.2 H2O 18 35 08.13234±0.00008 −07 35 04.1443±0.0012 125.0 8.17 122.2–127.0
VLBA DOY: 336 6.7 CH3OH 18 35 08.14234±0.00007 −07 35 03.9266±0.0010 115.4 2.59 109.8–120.2
12.2 CH3OH 18 35 08.13430±0.00006 −07 35 04.2821±0.0008 110.3 0.56 110.2–110.6
22.2 H2O 18 35 08.13233±0.00008 −07 35 04.1453±0.0012 124.8 9.39 122.1–127.1
LBA DOY: 271 6.7 CH3OH 18 35 08.14238±0.00009 −07 35 03.9259±0.0014 115.3 8.97 107.6–120.1
EVN DOY: 280 6.7 CH3OH 18 35 08.14231±0.00010 −07 35 03.9247±0.0010 115.2 7.34 108.1–120.2

Notes. (a) the coordinates taken from VLBA DOY: 300 (see Sect. 2.1 for details).

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