Free Access

Table 4

All 6.7 GHz methanol maser features detected in IRAS 18556+01 (G35.20–0.74N).

     (1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
Maser Group RA Dec Peak flux Vlsr ΔvL Pl χ ΔVia TbΔΩa ΔVZb θc
offset offset density(#I)
(mas) (mas) (Jy/beam) (km s-1) (km s-1) (%) (°) (km s-1) (log K sr) (m/s) (°)

I18556.01d A –1587.159 1817.554 14.71 ± 0.34 29.89 0.23 8.6 ± 1.3  −9 ± 3  <0.5  −
I18556.02 A –1563.866 1764.340 1.05 ± 0.10 28.57 0.42  −  −  −  −  −  −
I18556.03 A –1561.521 1881.611 0.85 ± 0.03 33.22 0.30  −  −  −  −  −  −
I18556.04d A –1558.818 1630.295 4.66 ± 0.03 36.56 0.26 9.1 ± 1.4 22 ± 28  <0.5  −
I18556.05 A –1559.276 1826.489 4.47 ± 0.03 27.95 0.24  −  −  −  −  −  −
I18556.06 A –1553.628 1790.443 0.32 ± 0.03 27.95 0.26  −  −  −  −  −  −
I18556.07 A –1551.154 1729.794 0.69 ± 0.02 27.60 0.28  −  −  −  −  −  −
I18556.08d A –1550.882 1862.656 12.13 ± 0.08 29.36 0.29 6.5 ± 0.7 2 ± 3  −
I18556.09 A –1549.567 1674.839 1.31 ± 0.02 30.41 0.30  −  −  −  −  −  −
I18556.10 A –1548.166 1827.927 0.52 ± 0.02 27.25 0.22  −  −  −  −  −  −
I18556.11 A –1548.080 1604.614 12.81 ± 0.11 35.42 0.30 4.8 ± 1.1 22 ± 18  −
I18556.12 A –1538.571 1715.225 0.14 ± 0.01 33.49 0.30  −  −  −  −  −  −
I18556.13 A –1535.311 1903.782 0.97 ± 0.03 33.22 0.20  −  −  −  −  −  −
I18556.14 A –1527.890 1870.255 0.56 ± 0.02 33.40 0.14  −  −  −  −  −  −
I18556.15 A –1519.568 1904.572 1.74 ± 0.01 26.90 0.43  −  −  −  −  −  −
I18556.16 A –1513.805 1912.239 1.36 ± 0.01 26.20 0.31  −  −  −  −  −  −
I18556.17 A –1501.437 1774.460 0.22 ± 0.01 30.94 0.21  −  −  −  −  −  −
I18556.18 A –1466.290 1754.551 0.20 ± 0.01 32.34 0.37  −  −  −  −  −  −
I18556.19 A –1454.021 1765.602 0.14 ± 0.01 31.73 0.27  −  −  −  −  −  −
I18556.20 A –1293.200 1994.118 4.37 ± 0.19 29.10 0.21  −  −  −  −  −  −
I18556.21 B –14.056 20.645 1.41 ± 0.02 27.95 0.40  −  −  −  −  −  −
I18556.22 B –14.013 28.847 3.86 ± 0.05 28.31 0.23  −  −  −  −  −  −
I18556.23 B –12.669 72.609 1.45 ± 0.05 28.31 0.65  −  −  −  −  −  −
I18556.24 B –11.039 17.769 0.39 ± 0.01 27.43 0.25  −  −  −  −  −  −
I18556.25 B –5.863 –4.211 0.31 ± 0.01 27.34 0.19  −  −  −  −  −  −
I18556.26 B –3.117 –277.435 1.58 ± 0.05 28.39 0.21  −  −  −  −  −  −
I18556.27d B 0 0 104.81 ± 1.05 28.57 0.26 11.5 ± 1.9  −10 ± 5  <0.5  −
I18556.28 B 49.389 48.145 0.89 ± 0.03 27.69 0.18  −  −  −  −  −  −

Notes. 

(a)

The best-fitting results obtained by using a model based on the radiative transfer theory of methanol masers for Γ + Γν = 1 (Vlemmings et al. 2010; Surcis et al. 2011b). The errors were determined by analyzing the full probability distribution function.

(b)

The Zeeman-splittings are determined from the cross-correlation between the RR and LL spectra.

(c)

The angle between the magnetic field and the maser propagation direction is determined by using the observed Pl and the fitted emerging brightness temperature. The errors were determined by analyzing the full probability distribution function.

(d)

Because of the degree of the saturation of these CH3OH masers TbΔΩ is underestimated, ΔVi and θ are overestimated.

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.