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Query : 2019A&A...626A..36D |
2019A&A...626A..36D - Astronomy and Astrophysics, volume 626A, 36-36 (2019/6-1)
ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19.
DALL'OLIO D., VLEMMINGS W.H.T., PERSSON M.V., ALVES F.O., BEUTHER H., GIRART J.M., SURCIS G., TORRELLES J.M. and VAN LANGEVELDE H.J.
Abstract (from CDS):
Abstract Copyright: © ESO 2019
Journal keyword(s): stars: formation - ISM: magnetic fields - magnetic fields - polarization - stars: massive
VizieR on-line data: <Available at CDS (J/A+A/626/A36): list.dat fits/*>
Simbad objects: 28
Number of rows : 28 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | QSO B1730-130 | QSO | 17 33 02.70578907 | -13 04 49.5482119 | 18 | 19.50 | 18.78 | 17.39 | ~ | 1140 | 1 | |
2 | 4C 09.57 | BLL | 17 51 32.81857326 | +09 39 00.7284066 | 17.46 | 16.78 | 15.57 | ~ | 948 | 1 | ||
3 | [GRM93] G09.61+0.20 A | Rad | 18 06 11.9 | -20 31 41 | ~ | 14 | 0 | |||||
4 | GAL 009.62+00.19 | HII | 18 06 13.9 | -20 31 44 | ~ | 209 | 0 | |||||
5 | [GRM93] G09.61+0.20 B | Rad | 18 06 14.1 | -20 31 43 | ~ | 18 | 0 | |||||
6 | [GRM93] G09.61+0.20 C | HII | 18 06 14.4 | -20 31 25 | ~ | 18 | 0 | |||||
7 | [LLL2017] MM1 | cor | 18 06 14.49 | -20 31 27.9 | ~ | 4 | 0 | |||||
8 | [LLL2017] MM2 | cor | 18 06 14.508 | -20 31 30.50 | ~ | 2 | 0 | |||||
9 | [LLL2017] MM4 | cor | 18 06 14.656 | -20 31 31.77 | ~ | 7 | 0 | |||||
10 | [GRM93] G09.61+0.20 E | HII | 18 06 14.7 | -20 31 32 | ~ | 46 | 0 | |||||
11 | [LLL2017] MM5 | cor | 18 06 14.705 | -20 31 12.63 | ~ | 2 | 0 | |||||
12 | [LLL2017] MM3 | cor | 18 06 14.758 | -20 31 30.13 | ~ | 2 | 0 | |||||
13 | [LLL2017] MM6 | cor | 18 06 14.781 | -20 31 34.85 | ~ | 4 | 0 | |||||
14 | [LLL2017] MM7 | cor | 18 06 14.798 | -20 31 37.21 | ~ | 5 | 0 | |||||
15 | [GRM93] G09.61+0.20 G | Rad | 18 06 14.805 | -20 31 37.17 | ~ | 10 | 0 | |||||
16 | [LLL2017] MM8 | cor | 18 06 14.852 | -20 31 39.54 | ~ | 6 | 0 | |||||
17 | [GRM93] G09.61+0.20 F | Rad | 18 06 14.89 | -20 31 38.9 | ~ | 29 | 1 | |||||
18 | [GRM93] G09.61+0.20 D | HII | 18 06 14.9 | -20 31 43 | ~ | 19 | 0 | |||||
19 | [LLL2017] MM10 | cor | 18 06 14.924 | -20 31 41.40 | ~ | 2 | 0 | |||||
20 | [LLL2017] MM11 | cor | 18 06 14.925 | -20 31 36.49 | ~ | 5 | 0 | |||||
21 | [LLL2017] MM9 | cor | 18 06 15.013 | -20 31 41.27 | ~ | 3 | 0 | |||||
22 | [LLL2017] MM12 | cor | 18 06 15.024 | -20 31 46.28 | ~ | 2 | 0 | |||||
23 | [GRM93] G09.61+0.20 H | Rad | 18 06 15.047 | -20 31 36.72 | ~ | 8 | 0 | |||||
24 | [GRM93] G09.61+0.20 I | Rad | 18 06 15.172 | -20 31 37.97 | ~ | 7 | 0 | |||||
25 | GAL 012.89+00.49 | HII | 18 11 51.3 | -17 31 29 | ~ | 184 | 0 | |||||
26 | QSO J1832-2039 | BLL | 18 32 11.0455806144 | -20 39 48.210054948 | 18.56 | 20.2 | ~ | 70 | 1 | |||
27 | QSO B1921-293 | BLL | 19 24 51.05595254 | -29 14 30.1210248 | 18.71 | 18.21 | 15.07 | ~ | 871 | 0 | ||
28 | DR 21 (OH) | cor | 20 39 01.01 | +42 22 50.2 | ~ | 410 | 0 |
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