2011A&A...529A.159G


C.D.S. - SIMBAD4 rel 1.7 - 2019.11.20CET19:38:15

2011A&A...529A.159G - Astronomy and Astrophysics, volume 529A, 159-159 (2011/5-1)

A Sino-German λ6 cm polarization survey of the Galactic plane. V. Large supernova remnants.

GAO X.Y., HAN J.L., REICH W., REICH P., SUN X.H. and XIAO L.

Abstract (from CDS):

Observations of large supernova remnants (SNRs) at high frequencies are rare, but provide valuable information about their physical properties. The total intensity and polarization properties of 16 large SNRs in the Galactic plane are investigated based on observations of the Urumqi λ6cm polarization survey of the Galactic plane with an angular resolution of 9.5'. We extracted total intensity and linear polarization maps of large SNRs from the Urumqi λ6cm survey, obtained their integrated flux densities, and derived the radio spectra by using these flux densities together with previously published flux densities at various frequencies. In particular, Effelsberg λ11cm and λ21cm survey data were used to calculate integrated flux densities. The λ6cm polarization data also delineate the magnetic field structures of the SNRs. We present the first total intensity maps at λ6cm for SNRs G106.3+2.7, G114.3+0.3, G116.5+1.1, G166.0+4.3 (VRO 42.05.01), G205.5+0.5 (Monoceros Nebula), and G206.9+2.3 (PKS 0646+06) and the first polarization measurements at λ6cm for SNRs G82.2+5.3 (W63), G106.3+2.7, G114.3+0.3, G116.5+1.1, G166.0+4.3 (VRO 42.05.01), G205.5+0.5 (Monoceros Nebula), and G206.9+2.3 (PKS 0646+06). Most of the newly derived integrated radio spectra are consistent with previous results. The new flux densities obtained from the Urumqi λ6cm, Effelsberg λ11cm and λ21cm surveys are crucial to determine the spectra of SNR G65.1+0.6, G69.0+2.7 (CTB 80), G93.7-0.2, and G114.3+0.3. We find that G192.8-1.1 (PKS 0607+17) consists of background sources, H ii regions, and extended diffuse emission of thermal nature, and conclude that G192.8-1.1 is not a SNR.

Abstract Copyright:

Journal keyword(s): ISM: supernova remnants - radio continuum: ISM - polarization - techniques: polarimetric

CDS comments: Paragraph 3.16 extended nebula 0641+06 is LBN 206.29+01.55 in Simbad

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 - 2020
#notes
1 SNR G126.2+01.6 SNR 01 22.0 +64 15           ~ 46 0
2 SNR G127.1+00.5 SNR 01 28 20.000 +63 10 00.00           ~ 84 0
3 3C 48 QSO 01 37 41.2995845985 +33 09 35.079126038   16.62 16.20     ~ 2432 2
4 SNR G130.7+03.1 SNR 02 05 37.0 +64 49 42           ~ 553 4
5 SNR G132.6+01.5 SNR 02 17 40 +62 45.0           ~ 153 0
6 SNR G156.2+05.7 SNR 04 58 51.300 +51 50 28.00           ~ 107 1
7 SNR G160.8+02.6 SNR 05 01 00.000 +46 40 00.00           ~ 184 0
8 SNR G166.2+02.5 SNR 05 19.0 +41 53           ~ 70 0
9 ICRF J052109.8+163822 Sy1 05 21 09.88592749 +16 38 22.0517668   19.37 18.84 18.480   ~ 726 1
10 2FGL J0526.6+4308 Bla 05 26 30.000 +42 56 00.00           ~ 150 0
11 SNR G180.0-01.7 SNR 05 39 00.000 +27 50 00.00           ~ 197 2
12 4C 31.21 Rad 05 53 21.60 +31 17 50.0           ~ 10 1
13 SNR G179.0+02.6 SNR 05 53.7 +31 05           ~ 28 0
14 NAME Lower's Nebula HII 06 08 44 +15 40.5           ~ 32 0
15 PKS 0607+17 Rad 06 09.3 +17 20           ~ 45 1
16 4C 16.15 Rad 06 09 33.50 +16 22 07.0           ~ 11 2
17 NVSS J060951+172532 Rad 06 09 51.20 +17 25 33.0           ~ 3 1
18 SH 2-259 HII 06 11 25.80 +17 26 25.0           ~ 31 1
19 LBN 192.48-00.21 HII 06 11 59 +18 03.3           ~ 84 0
20 NAME Origem Loop SNR 06 17 +16.1           ~ 13 0
21 2XMM J061705.2+222129 XB* 06 17 05.26 +22 21 29.4           ~ 42 1
22 IC 443 SNR 06 18 02.7 +22 39 36           ~ 1073 1
23 SNR G189.6+03.3 SNR 06 19 +22.2           ~ 25 0
24 LBN 188.69+04.25 HII 06 22 32 +22 58.5           ~ 41 1
25 NAME Rosette Nebula HII 06 31 40 +04 57.8           ~ 430 1
26 NAME Monoceros SNR SNR 06 38 43 +06 30.2           ~ 207 0
27 NGC 2264 OpC 06 40 58 +09 53.7     3.9     ~ 1547 1
28 LBN 206.29+01.55 HII 06 45 +06.6           ~ 2 0
29 SNR G206.9+02.3 SNR 06 48 40 +06 26.0           ~ 40 0
30 87GB 064656.6+054229 BLL 06 49 35.80 +05 38 23.2           ~ 3 1
31 3C 286 Sy1 13 31 08.2885060664 +30 30 32.960825108   17.51 17.25     ~ 3620 1
32 SNR G013.3-01.3 SNR 18 19 34 -18 00.0           ~ 18 0
33 SNR G028.8+01.5 Rad 18 39 00.000 -03 00 00.00           ~ 23 1
34 SNR G043.9+01.6 SNR 19 05.8 +10 30           ~ 27 0
35 SNR G032.0-04.9 SNR 19 06.0 -03 00           ~ 33 0
36 SS 433 HXB 19 11 49.5645897701 +04 58 57.824087535   16.3 13.0     A7Ib: 1898 3
37 SNR G039.7-02.0 SNR 19 12 20 +04 55.0           ~ 306 1
38 SNR G065.2+05.7 SNR 19 33.0 +31 10           ~ 84 0
39 SNR G068.8+02.6 SNR 19 52 55 +32 54.2           ~ 327 1
40 PSR B1951+32 Psr 19 52 58.181 +32 52 40.98           ~ 548 2
41 SNR G065.1+00.6 SNR 19 54.7 +28 35           ~ 41 0
42 IC 1318 HII 20 16 48 +41 57.4           ~ 42 0
43 SNR G078.3+02.5 SNR 20 18.6 +40 54           ~ 3 0
44 SNR G082.2+05.3 SNR 20 19.0 +45 30           ~ 84 0
45 NAME gam Cyg SNR SNR 20 20 17.100 +40 26 09.00           ~ 196 2
46 NAME Cyg X Cld 20 28 41 +41 10.2           ~ 589 1
47 NAME Cyg Complex reg 20 32 +45.0           ~ 508 0
48 SNR G089.0+04.7 SNR 20 45.0 +50 35           ~ 191 0
49 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 808 0
50 SNR G093.7-00.2 SNR 21 29.3 +50 50           ~ 60 1
51 SNR G106.3+02.7 SNR 22 27.5 +60 50           ~ 35 1
52 NAME Boomerang PWN G106.6+2.9 SNR 22 29 +61.2           ~ 29 1
53 SNR G108.2-00.6 SNR 22 53 37.0 +58 51 36           ~ 13 0
54 SH 2-147 HII 22 55.7 +58 28           ~ 40 1
55 PSR B2334+61 Psr 23 37 05.779 +61 51 01.69           ~ 165 1
56 SNR G114.3+00.3 SNR 23 37 05.780 +61 51 01.69           ~ 105 1
57 LBN 114.55+00.22 HII 23 39.8 +61 56           ~ 36 0
58 SNR G116.5+01.1 SNR 23 53 42.000 +63 15 00.00           ~ 58 0

    Equat.    Gal    SGal    Ecl

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2019.11.20-19:38:15

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