2021MNRAS.506.2232U


Query : 2021MNRAS.506.2232U

2021MNRAS.506.2232U - Mon. Not. R. Astron. Soc., 506, 2232-2246 (2021/September-2)

A first glimpse at the Galactic plane with the ASKAP: the SCORPIO field.

UMANA G., TRIGILIO C., INGALLINERA A., RIGGI S., CAVALLARO F., MARVIL J., NORRIS R.P., HOPKINS A.M., BUEMI C.S., BUFANO F., LETO P., LORU S., BORDIU C., BUNTON J.D., COLLIER J.D., FILIPOVIC M., FRANZEN T.M.O., THOMPSON M.A., ANDERNACH H., CARRETTI E., DAI S., KAPINSKA A., KORIBALSKI B.S., KOTHES R., LEAHY D., McCONNELL D., TOTHILL N. and MICHALOWSKI M.J.

Abstract (from CDS):

In the broad context of the Australian Square Kilometer Array Pathfinder (ASKAP) early-science phase and preparation for the related surveys, we report the first radio observations towards the Galactic plane. The targeted field was chosen to encompass the entire SCORPIO survey, one of the several pathfinder projects for the Evolutionary Map of the Universe survey planned with the ASKAP. The observations were carried out in 2018 January at a central frequency of 912 MHz, with 15 operational antennas, and covered a total area of about 40 square degrees in three different pointings. The final image has a resolution of 24.1 x 21.1 arcsec2 and a median rms of 541 µJy beam–1. We were able to extract 3545 candidate sources, 75 per cent of them point sources. For a preliminary validation, a comparison with the 843 MHz Molonglo Galactic Plane Survey is presented. Although the present observations were obtained with the ASKAP only partially deployed, its unique capability to map complex sources, such as those inhabiting the Galactic plane, at different angular scales, is highlighted. Within the SCORPIO field all the previously classified H II regions, Planetary Nebulae (PNe), and supernovae remnants (SNRs), previously known to be radio sources, were detected. We also report new radio detections from several H II regions previously classified as 'candidates' or 'radio quiet' and from half of all the PNe in the SCORPIO field with robust classification. Most notably, we find numerous unclassified, extended sources which constitute a promising sample of candidates H II regions and SNRs.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): techniques: image processing - techniques: interferometric - surveys - stars: evolution - stars: formation - radio continuum: general

VizieR on-line data: <Available at CDS (J/MNRAS/506/2232): table2.dat>

Status at CDS : Examining the need for a new acronym.

CDS comments: Table 4: SNR G345.1+0.2 and SNR G345.1-0.2 not identified.

Simbad objects: 58

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Number of rows : 58
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 PN G341.7+02.6 PN 16 42 18.6 -42 14 45           ~ 5 1
2 PN SuWt 3 PN 16 44 24.126 -40 03 20.60   20       ~ 30 0
3 SNR G340.4+00.4 SNR 16 46.5 -44 39           ~ 39 0
4 SNR G341.2+00.9 SNR 16 47.6 -43 47           ~ 34 1
5 SNR G340.6+00.3 SNR 16 47.7 -44 34           ~ 39 0
6 ESO 332-2 PN 16 49 32.85 -39 21 09.1           ~ 33 0
7 PN G344.0+02.5 PN 16 50 20.22 -40 30 03.1           ~ 9 1
8 PN Vd 4 PN 16 50 25.3507823664 -39 08 19.095453096     15.50     ~ 37 0
9 SNR G342.1+00.9 SNR 16 50.7 -43 04           ~ 19 0
10 ESO 332-4 PN 16 51 33.575 -40 02 56.01           ~ 28 0
11 NAME Sco OB 1 As* 16 53.5 -41 57           ~ 222 0
12 PN H 1-3 PN 16 53 31.33 -42 39 22.8     14.00     ~ 46 0
13 PN G343.5+01.2 PN 16 53 55.3 -41 44 00           ~ 8 1
14 PN Vd 6 PN 16 54 27.36 -38 44 10.5     17.70     ~ 30 0
15 PN G344.4+01.8 PN? 16 54 43.29 -40 41 46.9           ~ 13 1
16 SNR G342.0-00.2 SNR 16 54.8 -43 53           ~ 34 0
17 PN G343.6+01.1 PN? 16 54 51.0 -41 43 50           ~ 9 1
18 SNR G341.9-00.3 SNR 16 55.0 -44 01           ~ 42 0
19 PN G344.2+01.6 PN 16 55 00.50 -40 55 35.8           ~ 8 0
20 PN G345.8+02.7 PN 16 55 52.0032767832 -39 00 21.521254464           ~ 7 1
21 IRAS 16529-4341 PN 16 56 33.97296 -43 46 14.7468           ~ 18 0
22 PN G345.8+02.4 PN 16 56 40.118 -39 12 36.97           ~ 7 1
23 HD 152723 SB* 16 56 54.6694171728 -40 30 44.442698436 6.43 7.24 7.10 8.11 8.47 O6.5III(f) 163 0
24 PN H 1-5 PN 16 57 23.7543947808 -41 37 58.216237068     15.00     ~ 46 0
25 GAL 343.49-00.03 bub 16 59 20.8 -42 34 42           ~ 20 0
26 SCO J165948-420527 Rad 16 59 48.0 -42 05 27           ~ 1 0
27 SNR G343.1-00.7 SNR 17 00.4 -43 14           ~ 22 0
28 SCO J170029-421309 Rad 17 00 29.0 -42 13 09           ~ 1 0
29 SCO J170105-420531 Rad 17 01 05.0 -42 05 31           ~ 1 0
30 GAL 345.5+01.0 MoC 17 02 -40.3           ~ 8 0
31 SNR G344.7-00.1 SNR 17 03 49 -41 42.5           ~ 97 0
32 IC 4637 PN 17 05 10.47 -40 53 07.7     9.20     ~ 139 0
33 ESO 278-1 PN 17 05 38.3 -43 56 18           ~ 20 0
34 NAME Kn 98 PN? 17 06 19.600 -43 15 33.00           ~ 2 0
35 PN Pe 1-8 PN 17 06 22.49 -44 13 09.4     14.00     ~ 39 0
36 PN G342.7-02.3 PN 17 06 49.3 -44 34 35           ~ 5 1
37 PN H 1-6 PN 17 06 59.0827919760 -42 41 08.472952788     15.00     ~ 34 0
38 SNR G345.7-00.2 Rad 17 07.3 -40 53           ~ 23 1
39 WRAY 16-251 PN? 17 07 30.6034509216 -44 22 50.343108168     17.50   17.23 ~ 14 0
40 PN G343.9-01.6 PN 17 07 57.1502201496 -43 09 05.791878828           ~ 7 1
41 SNR G343.1-02.3 SNR 17 08.0 -44 16           ~ 82 1
42 PN G347.0+00.3 PN 17 09 10.8 -39 31 06           ~ 10 1
43 RCW 117 HII 17 09 34.0 -41 36 12           ~ 70 2
44 SNR G346.6-00.2 SNR 17 10.3 -40 11           ~ 99 0
45 PN H 1-7 PN 17 10 27.3823210128 -41 52 49.392533604   15.028 13.421 14.078   ~ 52 0
46 PN RPZM 3 PN? 17 11 25.4 -39 29 53           ~ 10 1
47 IRAS 17088-4227 PN 17 12 22.0468828848 -42 30 41.486666220           ~ 17 0
48 SNR G347.3-00.5 SNR 17 12 27 -39 41.2     12.27     ~ 761 1
49 PN G346.8-00.7 PN 17 13 10.841 -40 15 56.21           ~ 9 1
50 NAME Kn 102 PN? 17 14 25.000 -41 44 34.00           ~ 2 0
51 SNR G348.5+00.1 SNR 17 14 31.780 -38 28 34.50           ~ 233 3
52 PN G347.2-00.8 PN 17 14 49.1945959824 -40 06 07.367107860           ~ 11 1
53 PN G344.8-02.6 PN 17 15 15.9 -43 03 54           ~ 8 1
54 SNR G348.5-00.0 Rad 17 15 26 -38 28.0           ~ 39 1
55 NAME CBF-3 PN? 17 15 46.800 -42 24 06.12           ~ 1 0
56 IRAS 17123-3929 mul 17 15 47.7 -39 33 03           ~ 6 0
57 PN PM 1-135 PN 17 15 51.60336 -39 33 08.7984           ~ 6 0
58 ICRF J193925.0-634245 Sy2 19 39 25.0245304992 -63 42 45.640373400   18.87 18.37 17.64   ~ 1332 2

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