2017ApJ...849..140X


Query : 2017ApJ...849..140X

2017ApJ...849..140X - Astrophys. J., 849, 140-140 (2017/November-2)

Two-dimensional molecular gas and ongoing star formation around H II region Sh2-104.

XU J.-L., XU Y., YU N., ZHANG C.-P., LIU X.-L., WANG J.-J., NING C.-C., JU B.-G. and ZHANG G.-Y.

Abstract (from CDS):

We performed a multi-wavelength study toward H II region Sh2-104. New maps of 12CO J = 1 - 0 and 13CO J = 1 - 0 were obtained from the Purple Mountain Observatory 13.7 m radio telescope. Sh2-104 displays a double-ring structure. The outer ring with a radius of 4.4 pc is dominated by 12, 500 µm, 12CO J = 1 - 0, and 13CO J = 1 - 0 emission, while the inner ring with a radius of 2.9 pc is dominated by 22 µm and 21 cm emission. We did not detect CO emission inside the outer ring. The north-east portion of the outer ring is blueshifted, while the south-west portion is redshifted. The present observations have provided evidence that the collected outer ring around Sh2-104 is a two-dimensional structure. From the column density map constructed by the Hi-GAL survey data, we extract 21 clumps. About 90% of all the clumps will form low-mass stars. A power-law fit to the clumps yields M=281 M☉(r/pc)^1.31±0.08^. The selected YSOs are associated with the collected material on the edge of Sh2-104. The derived dynamical age of Sh2-104 is 1.6×106 yr. Comparing the Sh2-104 dynamical age with the YSO timescale and the fragmentation time of the molecular ring, we further confirm that the collect-and-collapse process operates in this region, indicating positive feedback from a massive star for surrounding gas.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): H II regions - ISM: clouds - stars: early-type - stars: formation - stars: formation

Nomenclature: Table 2: [XXY2017] NN (Nos 1-21).

Simbad objects: 34

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Number of rows : 34
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SH 2-212 HII 04 40 36.52 +50 27 44.3           ~ 102 2
2 LBN 159.17+03.33 HII 04 58 45.7 +47 59 36           ~ 86 1
3 IC 2599 HII 10 37.7 -58 39           ~ 48 2
4 GRS G308.60 +00.60 HII 13 39.9 -61 45           ~ 108 0
5 SH 2-3 HII 17 12.4 -38 28           ~ 234 1
6 [ABB2014] WISE G012.523-00.611 bub 18 15 04.8 -18 22 24           ~ 14 0
7 [L89b] 28.823-00.226 bub 18 44 44.3 -03 45 34           ~ 80 0
8 [ABB2014] WISE G034.158+00.147 bub 18 53 10 +01 09.2           ~ 14 0
9 [WBN74] W 51 IRS 2 SFR 19 23 39.93 +14 31 09.4           ~ 321 0
10 SH 2-87 bub 19 46 20.69 +24 35 15.4           ~ 161 2
11 LBN 063.10+00.46 HII 19 49 11.7 +26 51 36   14.60 13.63     ~ 55 0
12 [XXY2017] 16 MoC 20 17 27.30 +36 45 02.7           ~ 1 0
13 [XXY2017] 20 MoC 20 17 27.60 +36 46 08.9           ~ 1 0
14 [XXY2017] 13 MoC 20 17 29.20 +36 47 15.2           ~ 1 0
15 [XXY2017] 14 MoC 20 17 30.90 +36 43 15.0           ~ 1 0
16 [XXY2017] 21 MoC 20 17 32.70 +36 44 53.1           ~ 1 0
17 [XXY2017] 7 MoC 20 17 32.70 +36 47 57.3           ~ 1 0
18 [XXY2017] 11 MoC 20 17 34.50 +36 49 09.7           ~ 1 0
19 [XXY2017] 5 MoC 20 17 37.60 +36 42 29.3           ~ 1 0
20 [XXY2017] 2 MoC 20 17 42.50 +36 42 25.5           ~ 1 0
21 [XXY2017] 18 MoC 20 17 43.00 +36 41 32.4           ~ 1 0
22 JCMTSE J201745.7+364244 MoC 20 17 45.7 +36 42 44           ~ 2 0
23 [XXY2017] 17 MoC 20 17 45.80 +36 49 13.5           ~ 1 0
24 [XXY2017] 19 MoC 20 17 49.50 +36 42 29.3           ~ 1 0
25 JCMTSE J201749.6+364826 MoC 20 17 49.6 +36 48 26           ~ 2 0
26 SH 2-104 HII 20 17 52.5 +36 49 24           ~ 97 0
27 [XXY2017] 4 MoC 20 17 53.00 +36 45 04.9           ~ 1 0
28 [XXY2017] 15 MoC 20 17 54.10 +36 48 03.0           ~ 1 0
29 [XXY2017] 10 MoC 20 17 54.40 +36 43 40.1           ~ 1 0
30 [XXY2017] 1 MoC 20 17 54.70 +36 45 38.5           ~ 1 0
31 [XXY2017] 3 MoC 20 17 55.90 +36 44 45.7           ~ 1 0
32 IRAS 20160+3636 HII 20 17 56.1 +36 45 33           ~ 21 0
33 [XXY2017] 8 MoC 20 17 57.10 +36 46 32.8           ~ 1 0
34 [XXY2017] 12 MoC 20 17 57.40 +36 45 42.4           ~ 1 0

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