2013MNRAS.434..123V


Query : 2013MNRAS.434..123V

2013MNRAS.434..123V - Mon. Not. R. Astron. Soc., 434, 123-141 (2013/September-1)

Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models.

VIGANO D., REA N., PONS J.A., PERNA R., AGUILERA D.N. and MIRALLES J.A.

Abstract (from CDS):

Observations of magnetars and some of the high magnetic field pulsars have shown that their thermal luminosity is systematically higher than that of classical radio-pulsars, thus confirming the idea that magnetic fields are involved in their X-ray emission. Here we present the results of 2D simulations of the fully coupled evolution of temperature and magnetic field in neutron stars, including the state-of-the-art kinetic coefficients and, for the first time, the important effect of the Hall term. After gathering and thoroughly re-analysing in a consistent way all the best available data on isolated, thermally emitting neutron stars, we compare our theoretical models to a data sample of 40 sources. We find that our evolutionary models can explain the phenomenological diversity of magnetars, high-B radio-pulsars, and isolated nearby neutron stars by only varying their initial magnetic field, mass and envelope composition. Nearly all sources appear to follow the expectations of the standard theoretical models. Finally, we discuss the expected outburst rates and the evolutionary links between different classes. Our results constitute a major step towards the grand unification of the isolated neutron star zoo.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): stars: magnetic field - stars: neutron - X-rays: stars

Simbad objects: 67

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Number of rows : 67
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 PSR J0007+7303 Psr 00 06 34.20 +73 11 06.6           ~ 163 1
2 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 246 1
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 10530 1
4 PSR J0100-7211 Psr 01 00 42.86 -72 11 33.3   17.69 17.82     B3V 92 0
5 PSR J0146+6145 Psr 01 46 22.21 +61 45 03.8   28.100 25.620     ~ 550 0
6 NAME Sgr J0418+5729 gam 04 18 33.867 +57 32 22.91           ~ 215 0
7 RX J0420.0-5022 N*? 04 20 02.2 -50 22 46     25.5     ~ 86 0
8 SNR G160.8+02.6 SNR 05 01 00.000 +46 40 00.00           ~ 206 0
9 2XMM J050106.5+451634 X 05 01 08.0 +45 16 31           ~ 119 0
10 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 16507 1
11 SNR J052559-660453 SNR 05 26 00.4 -66 05 02     12.71     ~ 429 2
12 PSR B0525-66 Psr 05 26 00.7 -66 04 35           ~ 534 1
13 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5102 0
14 PSR J0538+2813 Psr 05 38 25.06 +28 17 11.0           ~ 188 2
15 SNR G180.0-01.7 SNR 05 39 00.000 +27 50 00.00           ~ 239 2
16 NAME Geminga Psr 06 33 54.153 +17 46 12.91           ~ 1172 0
17 NAME MONOGEM SNR SNR 06 58 50 +13 55.9           ~ 98 0
18 PSR B0656+14 Psr 06 59 48.1960 +14 14 19.400   24.85 24.90     ~ 829 1
19 RX J0720.4-3125 N* 07 20 24.961 -31 25 50.21   26.1   27.0   ~ 294 0
20 PSR J0726-2612 Psr 07 26 08.12 -26 12 38.1           ~ 27 0
21 RX J0806.4-4123 N*? 08 06 23.0 -41 22 33           ~ 77 0
22 RX J0822.0-4300 X 08 22 26.84204 -43 10 26.2350           ~ 42 1
23 NAME Pup A SNR 08 24 07 -42 59.8           ~ 572 1
24 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1190 2
25 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2240 1
26 2E 2336 HXB 10 50 08.93 -59 53 19.9           Be 396 0
27 PSR B1055-52 Psr 10 57 59.0450 -52 26 56.330           ~ 706 0
28 PSR J1119-6127 Psr 11 19 14.30 -61 27 49.5           ~ 376 1
29 SNR G292.2-00.5 SNR 11 19.3 -61 28           ~ 88 1
30 SNR G295.5+09.7 SNR 12 09 40 -52 25.0           ~ 277 1
31 PSR J1210-5226 Psr 12 10 00.88 -52 26 28.4           ~ 223 1
32 RX J1308.8+2127 N*? 13 08 48.7 +21 27 08   28.6 28.6     ~ 152 1
33 PSR J1550-5418 Psr 15 50 54.18 -54 18 23.9           ~ 384 1
34 SNR G327.2-00.1 SNR 15 50 55 -54 18.0           ~ 64 1
35 RX J1605.3+3249 N*? 16 05 18.9 +32 49 07     26.8     ~ 97 1
36 SNR G337.0-00.1 SNR 16 35 06.9 -47 47 25           ~ 128 1
37 GRB 980618A gB 16 35 52 -47 35.2           ~ 257 0
38 Cl Westerlund 1 Cl* 16 47 04.00 -45 51 04.9           ~ 526 0
39 PSR J1647-4552 Psr 16 47 10.18 -45 52 16.7           ~ 193 1
40 PSR J1708-4008 Psr 17 08 49.0 -40 09 10           ~ 283 0
41 PSR B1706-44 Psr 17 09 42.7460 -44 29 07.200     13.30     ~ 618 1
42 SNR G348.7+00.3 SNR 17 13 43.0 -38 10 12           ~ 119 2
43 [AAB2008] 1 X 17 14 05.758 -38 10 31.32           ~ 57 1
44 PSR J1718-3718 Psr 17 18 10.16 -37 18 53.8           ~ 70 0
45 PSR J1740+1000 Psr 17 40 25.91 +10 00 06.0           ~ 74 0
46 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1199 2
47 AX J1809.8-1943 Psr 18 09 51.07 -19 43 51.8           ~ 435 0
48 W 31 SFR 18 10 28.6 -19 55 51           ~ 252 0
49 PSR J1819-1458 Psr 18 19 34.173 -14 58 03.57           ~ 114 0
50 1WGA J1822.2-1604 X 18 22 18.32 -16 04 27.2           ~ 125 0
51 NAME Sgr 1833-0832 gam 18 33 46.0 -08 32 13           ~ 76 0
52 SWIFT J1834.9-0846 N*? 18 34 52.768 -08 45 40.83           ~ 81 0
53 PSR J1841-0456 Psr 18 41 19.29 -04 56 11.4           ~ 257 1
54 4C -04.71 Rad 18 41 19.8 -04 56 06           ~ 318 3
55 PSR J1846-0258 Psr 18 46 24.94 -02 58 30.1           ~ 332 2
56 SNR G033.6+00.1 SNR 18 52 29.000 +00 38 42.00           ~ 273 1
57 PSR J1852+0040 Psr 18 52 38.49 +00 40 19.8           ~ 86 1
58 RX J1856.6-3754 Psr 18 56 35.11 -37 54 30.5     25.7     ~ 418 0
59 NAME Sgr 1900-14 Rad 19 03 32.80 -13 57 56.3           ~ 12 1
60 GBS 1900+14 gB 19 07 13 +09 19.6           ~ 832 0
61 RX J2143.0+0654 N*? 21 43 03.8 +06 54 20           ~ 75 0
62 2E 4673 HXB 23 01 08.14 +58 52 44.5           ~ 615 1
63 SNR G109.1-01.0 SNR 23 01 35 +58 53.0           ~ 335 0
64 NAME Cas A SNR 23 23 24.000 +58 48 54.00     14.30     ~ 2668 1
65 PSR B2334+61 Psr 23 37 05.779 +61 51 01.69           ~ 182 1
66 SNR G114.3+00.3 SNR 23 37 05.780 +61 51 01.69           ~ 117 1
67 NAME Sgr 1806-23 ? ~ ~           ~ 5 0

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2023.01.28-12:20:40

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