2018A&A...612A...2H


C.D.S. - SIMBAD4 rel 1.7 - 2021.03.08CET20:32:33

2018A&A...612A...2H - Astronomy and Astrophysics, volume 612A, 2-2 (2018/4-1)

The population of TeV pulsar wind nebulae in the H.E.S.S. Galactic Plane Survey.

HESS COLLABORATION, ABDALLA H., ABRAMOWSKI A., AHARONIAN F., AIT BENKHALI F., AKHPERJANIAN A.G., ANDERSSON T., ANGUNER E.O., ARRIETA M., AUBERT P., BACKES M., BALZER A., BARNARD M., BECHERINI Y., BECKER TJUS J., BERGE D., BERNHARD S., BERNLOHR K., BLACKWELL R., BOTTCHER M., BOISSON C., BOLMONT J., BORDAS P., BREGEON J., BRUN F., BRUN P., BRYAN M., BULIK T., CAPASSO M., CARR J., CARRIGAN S., CASANOVA S., CERRUTI M., CHAKRABORTY N., CHALME-CALVET R., CHAVES R.C.G., CHEN A., CHEVALIER J., CHRETIEN M., COLAFRANCESCO S., COLOGNA G., CONDON B., CONRAD J., COUTURIER C., CUI Y., DAVIDS I.D., DEGRANGE B., DEIL C., DEVIN J., DEWILT P., DIRSON L., DJANNATI-ATAI A., DOMAINKO W., DONATH A., DRURY L.O., DUBUS G., DUTSON K., DYKS J., EDWARDS T., EGBERTS K., EGER P., ERNENWEIN J.-P., ESCHBACH S., FARNIER C., FEGAN S., FERNANDES M.V., FIASSON A., FONTAINE G., FORSTER A., FUNK S., FUSSLING M., GABICI S., GAJDUS M., GALLANT Y.A., GARRIGOUX T., GIAVITTO G., GIEBELS B., GLICENSTEIN J.F., GOTTSCHALL D., GOYAL A., GRONDIN M.-H., HADASCH D., HAHN J., HAUPT M., HAWKES J., HEINZELMANN G., HENRI G., HERMANN G., HERVET O., HILLERT A., HINTON J.A., HOFMANN W., HOISCHEN C., HOLLER M., HORNS D., IVASCENKO A., JACHOLKOWSKA A., JAMROZY M., JANIAK M., JANKOWSKY D., JANKOWSKY F., JINGO M., JOGLER T., JOUVIN L., JUNG-RICHARDT I., KASTENDIECK M.A., KATARZYNSKI K., KATZ U., KERSZBERG D., KHELIFI B., KIEFFER M., KING J., KLEPSER S., KLOCHKOV D., KLUZNIAK W., KOLITZUS D., KOMIN N., KOSACK K., KRAKAU S., KRAUS M., KRAYZEL F., KRUGER P.P., LAFFON H., LAMANNA G., LAU J., LEES J.-P., LEFAUCHEUR J., LEFRANC V., LEMIERE A., LEMOINE-GOUMARD M., LENAIN J.-P., LESER E., LOHSE T., LORENTZ M., LIU R., LOPEZ-COTO R., LYPOVA I., MARANDON V., MARCOWITH A., MARIAUD C., MARX R., MAURIN G., MAXTED N., MAYER M., MEINTJES P.J., MEYER M., MITCHELL A.M.W., MODERSKI R., MOHAMED M., MOHRMANN L., MORA K., MOULIN E., MURACH T., DE NAUROIS M., NIEDERWANGER F., NIEMIEC J., OAKES L., O'BRIEN P., ODAKA H., OTTL S., OHM S., DE ONA WILHELMI E., OSTROWSKI M., OYA I., PADOVANI M., PANTER M., PARSONS R.D., PAZ ARRIBAS M., PEKEUR N.W., PELLETIER G., PERENNES C., PETRUCCI P.-O., PEYAUD B., PITA S., POON H., PROKHOROV D., PROKOPH H., PUHLHOFER G., PUNCH M., QUIRRENBACH A., RAAB S., REIMER A., REIMER O., RENAUD M., DE LOS REYES R., RIEGER F., ROMOLI C., ROSIER-LEES S., ROWELL G., RUDAK B., RULTEN C.B., SAHAKIAN V., SALEK D., SANCHEZ D.A., SANTANGELO A., SASAKI M., SCHLICKEISER R., SCHUSSLER F., SCHULZ A., SCHWANKE U., SCHWEMMER S., SETTIMO M., SEYFFERT A.S., SHAFI N., SHILON I., SIMONI R., SOL H., SPANIER F., SPENGLER G., SPIES F., STAWARZ L., STEENKAMP R., STEGMANN C., STINZING F., STYCZ K., SUSHCH I., TAVERNET J.-P., TAVERNIER T., TAYLOR A.M., TERRIER R., TIBALDO L., TIZIANI D., TLUCZYKONT M., TRICHARD C., TUFFS R., UCHIYAMA Y., VALERIUS K., VAN DER WALT D.J., VAN ELDIK C., VAN SOELEN B., VASILEIADIS G., VEH J., VENTER C., VIANA A., VINCENT P., VINK J., VOISIN F., VOLK H.J., VUILLAUME T., WADIASINGH Z., WAGNER S.J., WAGNER P., WAGNER R.M., WHITE R., WIERZCHOLSKA A., WILLMANN P., WORNLEIN A., WOUTERS D., YANG R., ZABALZA V., ZABOROV D., ZACHARIAS M., ZDZIARSKI A.A., ZECH A., ZEFI F., ZIEGLER A. and ZYWUCKA N.

Abstract (from CDS):

The nine-year H.E.S.S. Galactic Plane Survey (HGPS) has yielded the most uniform observation scan of the inner Milky Way in the TeV gamma-ray band to date. The sky maps and source catalogue of the HGPS allow for a systematic study of the population of TeV pulsar wind nebulae found throughout the last decade. To investigate the nature and evolution of pulsar wind nebulae, for the first time we also present several upper limits for regions around pulsars without a detected TeV wind nebula. Our data exhibit a correlation of TeV surface brightness with pulsar spin-down power E. This seems to be caused both by an increase of extension with decreasing E, and hence with time, compatible with a power law RPWN(E)∼E–0.65±0.20, and by a mild decrease of TeV gamma-ray luminosity with decreasing E, compatible with L1–10TeV∼E0.59±0.21. We also find that the offsets of pulsars with respect to the wind nebula centre with ages around 10kyr are frequently larger than can be plausibly explained by pulsar proper motion and could be due to an asymmetric environment. In the present data, it seems that a large pulsar offset is correlated with a high apparent TeV efficiency L1–10TeV/E. In addition to 14 HGPS sources considered firmly identified pulsar wind nebulae and 5 additional pulsar wind nebulae taken from literature, we find 10 HGPS sources that are likely TeV pulsar wind nebula candidates. Using a model that subsumes the present common understanding of the very high-energy radiative evolution of pulsar wind nebulae, we find that the trends and variations of the TeV observables and limits can be reproduced to a good level, drawing a consistent picture of present-day TeV data and theory.

Abstract Copyright: © ESO 2018

Journal keyword(s): gamma rays: general - catalogs - surveys - ISM: supernova remnants - pulsars: general

CDS comments: Table 4 HESS J1746-308 not in SIMBAD.

Simbad objects: 86

goto Full paper

goto View the reference in ADS

Number of rows : 86

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 238 1
2 3C 48 QSO 01 37 41.2995845985 +33 09 35.079126038   16.62 16.20     ~ 2566 2
3 SNR G130.7+03.1 SNR 02 05 37.0 +64 49 42           ~ 573 4
4 PSR J0205+6449 Psr 02 05 37.92 +64 49 42.8           ~ 215 1
5 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 15216 1
6 M 1 SNR 05 34 31.94 +22 00 52.2           ~ 5705 4
7 NGC 2060 SNR 05 37 51.4470067818 -69 10 23.957283532   9.69 9.59     ~ 327 2
8 NAME Geminga Psr 06 33 54.153 +17 46 12.91           ~ 1106 0
9 NAME Vela X Psr 08 33 08.880 -45 11 24.36           ~ 250 1
10 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1135 2
11 BRAN 226 HII 09 03 21.4 -48 25 48           ~ 18 0
12 PSR J1016-58 Psr 10 16 21.266 -58 57 11.70           ~ 92 3
13 HESS J1018-589 gam 10 18 -58.9           ~ 21 0
14 2FGL J1019.0-5856 HXB 10 19 02.270 -58 56 29.87           ~ 100 0
15 PSR J1023-5746 Psr 10 23 02.388 -57 46 09.86           ~ 49 0
16 FGES J1023.3-5747 gam 10 23 15.18313 -57 46 34.7840           ~ 53 0
17 Cl Westerlund 2 OpC 10 23 58.1 -57 45 49   11.59 10.5     ~ 294 0
18 PSR J1028-5819 Psr 10 28 27.888 -58 19 06.14           ~ 89 1
19 PSR J1055-6028 Psr 10 56 11.87 -60 27 12.7           ~ 29 1
20 PSR J1112-6103 Psr 11 12 14.81 -61 03 31.1           ~ 52 0
21 PSR J1119-6127 Psr 11 19 14.30 -61 27 49.5           ~ 341 1
22 SNR G292.2-00.5 SNR 11 19.3 -61 28           ~ 84 1
23 PSR J1124-5916 Psr 11 24 39.1 -59 16 20           ~ 136 1
24 PSR J1301-6305 Psr 13 01 45.76 -63 05 33.9           ~ 102 2
25 CPD-63 2495 HXB 13 02 47.6541729594 -63 50 08.625922862 10.34 10.72 9.98 10.03   O9.5Ve 689 1
26 PSR B1338-62 Psr 13 41 42.63 -62 20 20.7           ~ 113 1
27 PSR J1357-6429 Psr 13 57 02.525 -64 29 29.89           ~ 121 1
28 SNR G310.6-01.6 SNR 14 00 45.69 -63 25 42.6           ~ 27 1
29 PSR J1406-6121 Psr 14 06 50.04 -61 21 27.9           ~ 18 0
30 PSR J1410-6132 Psr 14 10 24.000 -61 32 00.00           ~ 114 1
31 PSR J1412-6145 Psr 14 12 07.69 -61 45 28.8           ~ 30 1
32 PSR J1413-6141 Psr 14 13 09.87 -61 41 13.0           ~ 29 1
33 AX J1418.7-6058 X 14 18 38.6 -60 57 49           ~ 44 0
34 PSR J1418-6058 Psr 14 18 42.725 -60 58 01.89           ~ 106 0
35 NAME Kookaburra reg 14 19 -60.9           ~ 48 1
36 PSR J1420-6048 Psr 14 20 08.190 -60 48 14.85           ~ 162 0
37 PSR J1459-60 Psr 14 59 30.222 -60 53 19.87           ~ 44 0
38 3A 1510-590 Psr 15 13 17.000 -59 04 54.00           ~ 382 3
39 PSR J1550-5418 Psr 15 50 54.18 -54 18 23.9           ~ 349 1
40 SNR G327.1-01.1 SNR 15 54 32.3 -55 03 44           ~ 86 1
41 AJG 44 Psr 16 17 33.000 -51 02 00.00           ~ 463 3
42 3EG J1639-4702 gam 16 40 30.0 -46 33 00           ~ 135 2
43 PSR J1640-4631 Psr 16 40 43.52 -46 31 35.4           ~ 41 0
44 PSR B1643-43 Psr 16 46 50.86 -43 45 53.7           ~ 59 1
45 PSR J1702-4310 Psr 17 02 26.94 -43 10 40.0           ~ 20 0
46 HESS J1708-443 gam 17 07 59.53847 -44 17 19.0460           ~ 12 0
47 SNR G348.5+00.1 SNR 17 14 31.780 -38 28 34.50           ~ 200 3
48 HESS J1718-385 gam 17 18 07 -38 33.0           ~ 30 0
49 2CG 359+00 gam 17 45 11 -30 11.9           ~ 91 0
50 GAL 000.0+00.0 gam 17 45 39.60213 -29 00 22.0000           ~ 12014 0
51 PSR B1742-30 Psr 17 45 56.3250 -30 40 22.600           ~ 145 0
52 SNR G000.9+00.1 SNR 17 47.3 -28 09           ~ 173 1
53 PSR B1757-24 Psr 18 01 00.016 -24 51 27.50           ~ 216 1
54 1AGLR J1807-2103 gam 18 04 29.70 -21 43 57.2           ~ 63 0
55 HESS J1809-193 gam 18 10 31 -19 18.0           ~ 44 1
56 NAME AGPS 273.4-17.8 SNR 18 13 35.05 -17 49 58.1           ~ 93 2
57 PSR J1815-1738 Psr 18 15 14.67 -17 38 03.0           ~ 20 0
58 SNR G015.4+00.1 Rad 18 18.0 -15 27           ~ 25 1
59 PSR J1826-1256 Psr 18 26 08.570 -12 56 33.53           ~ 103 1
60 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 359 1
61 HESS J1832-085 gam 18 32 -08.5           ~ 4 0
62 PSR J1832-0836 Psr 18 32 27.5940 -08 36 54.969           ~ 35 0
63 SNR G021.5-00.9 SNR 18 33 33.612 -10 34 07.69           ~ 401 1
64 PSR B1830-08 Psr 18 33 40.2640 -08 27 32.000           ~ 115 1
65 SNR G023.3-00.3 SNR 18 34 51.80 -08 44 38.2           ~ 194 0
66 PSR B1835-06.1 Psr 18 37 43.55 -06 04 49.0           ~ 50 0
67 PSR J1838-0655 Psr 18 38 03.13 -06 55 33.4           ~ 82 1
68 ARGO J1839-0627 Psr 18 40 55.0 -05 33 00           ~ 47 1
69 PSR J1841-0524 Psr 18 41 49.3551255320 -05 24 30.537633506           ~ 27 0
70 PSR J1846-0258 Psr 18 46 24.94 -02 58 30.1           ~ 305 2
71 SNR G029.7-00.2 SNR 18 46 25.5 -02 59 14           ~ 300 2
72 PSR J1849-0001 Psr 18 49 01.83 -00 01 19.1           ~ 39 0
73 PSR J1850-0026 Psr 18 50 14.714 -00 26 11.60           ~ 7 1
74 4FGL J1857.7+0246e Psr 18 57 11.0 +02 40 00           ~ 37 0
75 HESS J1858+020 gam 18 58 20.0 +02 05 24           ~ 36 0
76 PSR J1907+09 Psr 19 07 22.441 +09 18 30.76           ~ 26 0
77 ARGO J1907+0627 gam 19 08.7 +06 11           ~ 54 0
78 PSR J1909+0749 Psr 19 09 08 +07 49.6           ~ 6 0
79 SNR G054.1+00.3 SNR 19 30 31 +18 52.0           ~ 196 1
80 PSR B1930+22 Psr 19 32 22.8562490934 +22 20 52.062067050     14.52     ~ 119 0
81 PSR J1934+2352 Psr 19 34 46 +23 52.9           ~ 3 0
82 PSR J1935+2025 Psr 19 35 41.941 +20 25 40.10           ~ 17 0
83 SNR G076.9+01.0 SNR 20 22 20.000 +38 43 00.00           ~ 59 0
84 PSR J2022+3842 Psr 20 22 21.689 +38 42 14.82           ~ 35 0
85 PSR J2229+6114 Psr 22 29 05.262 +61 14 08.48           ~ 181 2
86 NAME Scutum Spiral Arm PoG ~ ~           ~ 290 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2018A&A...612A...2H and select 'bookmark this link' or equivalent in the popup menu


2021.03.08-20:32:33

© Université de Strasbourg/CNRS

    • Contact