EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 619 (November 2018) A&A, 619 (2018) A35 Full HTML
Free Access

Table C.1.

Luminosities of bright targets and of targets with broad maser lines.

ID Long AK(field) AK(tot) Mbol(kin) Mbol(14.5) Vlsr FWHM Comments References
(°) (mag) (mag) (mag) (mag) (km s−1) (km s−1)
436 29.85 0.12 ..0 .. −8.4 .. .. M3I (1)
444 29.67 1.16 0.88 .. −7.9 .. .. M2I (2)
483 29.26 1.32 1.40 −5.6 −7.1 66.9 4.3 RSGa (3)
535 24.63 1.29 1.76 .. −5.0 .. .. RSGa (4)
31 −0.44 1.80 1.72 .. −7.3 −24.4 9.6 Mbol(14.5) < −7.2, long < 5°
75 0.77 1.36 1.20 .. −8.0 −38.1 3.3 Mbol(14.5) < −7.2, long < 5°
92 0.11 1.66 1.41 .. −8.2 119.4 2.9 Mbol(14.5 ) < −7.2, long < 5°, sRSGb (5)
116 2.49 1.75 1.40 .. −7.6 19.5 4.2 Mbol(14.5) < −7.2, long < 5°
128 2.70 1.51 1.60 .. −7.9 −16.4 4.5 Mbol(14.5) < −7.2, long < 5°
294 −1.00 2.23 2.37 .. −7.8 .. .. Mbol(14.5) < −7.2, long < 5°, sRSGb (5)
310 −0.55 2.79 2.42 .. −7.4 .. .. Mbol(14.5) < −7.2, long < 5°
244 20.40 0.96 0.99 −6.2 −7.1 89.1 3.3 Mbol(kin) <  − 6.0, long > 20°
449 21.70 1.05 0.91 −6.3 −7.6 73.6 8.2 Mbol(kin) <  − 6.0, long > 20°
456 22.46 1.61 1.36 −6.6 −7.3 111.1 3.5 Mbol(kin) <  − 6.0, long > 20°
460 24.43 1.20 0.98 −6.2 −8.1 49.0 13.2 Mbol(kin) <  − 6.0, long > 20°
473 26.59 0.72 0.65 −6.1 −7.0 96.8 6.0 Mbol(kin) <  − 6.0, long > 20°
474 27.05 0.82 0.50 −6.4 −7.9 66.9 11.8 Mbol(kin) <  − 6.0, long > 20°
484 30.94 0.56 0.35 −6.3 −7.7 69.2 7.3 Mbol(kin) <  − 6.0, long > 20°
495 33.30 0.95 0.59 −6.1 −7.1 84.5 3.8 Mbol(kin) <  − 6.0, long > 20°
15 −1.38 0.99 0.89 −6.9 −7.2 38.7 7.3 Mbol(kin) <  − 6.0, long < 20°, FGc
23 −1.29 1.22 1.07 −6.8 −7.0 56.5 2.8 Mbol(kin) <  − 6.0, long < 20°, FGc
113 1.98 1.31 1.13 −6.7 −7.1 31.7 13.9 Mbol(kin) <  − 6.0, long < 20°, FGc
129 3.82 0.47 0.36 −7.1 −7.7 38.0 13.9 Mbol(kin) <  − 6.0, long < 20°, FGc
130 4.49 0.68 0.52 −6.4 −6.9 52.8 3.2 Mbol(kin) <  − 6.0, long < 20°, FGc
160 6.96 0.82 0.82 −6.2 −7.3 39.9 7.8 Mbol(kin) <  − 6.0, long < 20°, FGc
71 0.32 1.84 2.12 .. −5.3 92.5 9.0 Remaining FWHM > 9
87 1.24 1.21 1.24 .. −7.2 −15.3 9.2 Remaining FWHM > 9
117 2.01 1.85 3.25 .. −5.6 22.2 16.3 Remaining FWHM > 9
135 3.81 1.20 1.46 .. −5.6 207.1 11.9 Remaining FWHM > 9
173 8.66 1.61 1.20 .. −7.5 −1.1 11.5 Remaining FWHM > 9
190 10.99 1.04 1.10 .. −6.4 58.1 9.1 Remaining FWHM > 9
203 14.31 0.91 3.14 .. −4.0 81.1 12.7 Remaining FWHM > 9
223 17.80 1.02 1.87 .. −5.2 143.9 13.4 Remaining FWHM > 9
232 17.92 1.10 1.45 .. −5.4 94.3 9.8 Remaining FWHM > 9
452 21.71 1.11 1.54 −5.7 −6.6 97.1 13.3 Remaining FWHM > 9
457 22.25 1.51 1.28 −4.3 −7.5 19.8 9.1 Remaining FWHM > 9
459 24.13 1.05 1.66 −5.5 −5.6 139.5 10.4 Remaining FWHM > 9
469 25.97 0.86 1.70 −4.3 −4.9 113.4 12.7 Remaining FWHM > 9
481 29.12 0.73 0.31 −3.2 −7.8 10.2 11.7 Remaining FWHM > 9
486 31.67 1.75 5.20 −4.2 −5.2 91.0 10.6 Remaining FWHM > 9
489 31.50 1.43 2.68 −4.7 −5.4 98.0 9.8 Remaining FWHM > 9
490 31.36 1.55 2.27 −4.0 −5.5 69.8 12.4 Remaining FWHM > 9
491 33.42 1.11 1.09 −4.2 −7.0 31.5 14.6 Remaining FWHM > 9
493 34.00 1.04 1.38 −5.0 −6.1 78.9 11.1 Remaining FWHM > 9
502 35.06 2.02 2.02 −5.4 −7.5 45.8 9.1 Remaining FWHM > 9
511 35.25 1.47 2.49 −0.9 −6.2 7.3 9.2 Remaining FWHM > 9
526 44.24 0.94 1.39 −3.2 −5.7 34.0 9.7 Remaining FWHM > 9
530 47.95 0.71 1.88 −4.0 −4.8 58.0 10.4 Remaining FWHM > 9
432 28.97 0.97 1.17 −5.4 −6.2 103.1 19.9 Remaining FWHM > 9

Notes. Identification numbers (ID) are followed by longitudes (Long), median extinction of surrounding stars AK(field), total extinction of the targets AK(tot) (Messineo et al. 2005), Mbol values obtained by adopting the near kinematic distances, Mbol(kin), Mbol values obtained by adopting a distance modulus of 14.5 mag, radial velocities, Vlsr, and the maser line FWHMs. References. 1 = Jura & Kleinmann (1990) ; 2 = Messineo et al. (2016); 3 = Clark et al. (2009); 4 = Negueruela et al. (2010); 5 = this work.

(a)

RSG = Star photometrically reported as a probable RSG in previous studies.

(b)

sRSG = Stars confirmed as RSGs in this work with the spectral indexes of Messineo et al. (2017).

(c)

FG = Stars classified as likely foreground by Messineo et al. (2005), their AKs values are smaller than the average AKs of surrounding stars.

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.