2019MNRAS.485.5394K


C.D.S. - SIMBAD4 rel 1.7 - 2020.10.19CEST18:26:27

2019MNRAS.485.5394K - Mon. Not. R. Astron. Soc., 485, 5394-5410 (2019/June-1)

Stellar binaries that survive supernovae.

KOCHANEK C.S., AUCHETTL K. and BELCZYNSKI K.

Abstract (from CDS):

The number of binaries containing black holes (BH) or neutron stars (NS) depends critically on the fraction of binaries that survive supernova (SN) explosions. We searched for surviving star plus remnant binaries in a sample of 49 supernova remnants (SNR) containing 23 previously identified compact remnants and three high-mass X-ray binaries (HMXB), finding no new interacting or non-interacting binaries. The upper limits on any main-sequence stellar companion are typically ≲0.2 M_☉and are at worst ≲3 M_☉. This implies that f < 0.1 of core-collapse SNRs contain a non-interacting binary, and f = 0.083 (0.032 < f < 0.17) contain an interacting binary at 90 per cent confidence. We also find that the transverse velocities of HMXBs are low, with a median of only 12 km s–1 for field HMXBs, so surviving binaries will generally be found very close to the explosion centre. We compare the results to a 'standard' StarTrack binary population synthesis (BPS) model, finding reasonable agreement with the observations. In particular, the BPS models predict that 6 per cent of initial binaries leave a star plus remnant binary, or 5 per cent of SNRs assuming an 84 per cent binary fraction.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: binaries - stars: massive - supernovae: general

Status at CDS : Tables of objects will be appraised for possible ingestion in SIMBAD.

CDS comments: SNR G343.0-0.60 is not in Simbad (not enough information) // In table 3, the IDs Gaia DR2 620657678322625920 and 84497471323752064 are erroneous; they do not exist in Gaia DR2.

Simbad objects: 118

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Number of rows : 118

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 TYC 4018-3227-1 * 00 02 55.7097176984 +62 46 17.666764800   12.49 11.67     ~ 36 1
2 PSR J0007+7303 Psr 00 06 34.20 +73 11 06.6           ~ 149 1
3 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 236 1
4 SN 1572A SN* 00 25 21.5 +64 08 27           B8 1079 1
5 SNR G127.1+00.5 SNR 01 28 20.000 +63 10 00.00           ~ 90 0
6 EM* GGA 104 HXB 01 47 00.2121223849 +61 21 23.661992704 11.76 12.09 11.366 11.00 10.52 B1IIIe 172 0
7 SNR G130.7+03.1 SNR 02 05 37.0 +64 49 42           ~ 568 4
8 PSR J0205+6449 Psr 02 05 37.92 +64 49 42.8           ~ 212 1
9 PSR J0215+6218 Psr 02 15 56.626 +62 18 33.37           ~ 14 0
10 SNR G132.6+01.5 SNR 02 17 40 +62 45.0           ~ 158 0
11 LS I +61 303 HXB 02 40 31.6641883136 +61 13 45.591138110 11.27 11.61 10.75 10.19 9.55 B0Ve 765 2
12 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 5755 1
13 V* X Per HXB 03 55 23.0778791365 +31 02 45.045745259 6.090 6.840 6.720     O9.5III 908 0
14 SNR G156.2+05.7 SNR 04 58 51.300 +51 50 28.00           ~ 112 1
15 SNR G160.8+02.6 SNR 05 01 00.000 +46 40 00.00           ~ 192 0
16 2XMM J050106.5+451634 X 05 01 08.0 +45 16 31           ~ 106 0
17 PSR B0458+46 Psr 05 02 04.561 +46 54 06.09           ~ 76 0
18 HD 34921 HXB 05 22 35.2312215793 +37 40 33.640277173 6.78 7.64 7.48     B0IVpe 115 0
19 2FGL J0526.6+4308 Bla 05 26 30.000 +42 56 00.00           ~ 158 0
20 V* CM Tau Psr 05 34 31.93830 +22 00 52.1758           ~ 4828 1
21 M 1 SNR 05 34 31.94 +22 00 52.2           ~ 5647 4
22 SN 1987A SN* 05 35 28.020 -69 16 11.07           SNIIpec 4522 2
23 PSR J0538+2813 Psr 05 38 25.06 +28 17 11.0           ~ 167 2
24 HD 245770 HXB 05 38 54.5749436467 +26 18 56.839215267 9.30 9.84 9.39 8.77 8.30 O9/B0III/Ve 878 0
25 SNR G180.0-01.7 SNR 05 39 00.000 +27 50 00.00           ~ 215 2
26 HD 37424 * 05 39 44.4007611413 +27 46 51.190285913   9.05 8.99     B9 13 0
27 HD 249179 HXB 05 55 55.0408711373 +28 47 06.429887265   10.11 10.00     B5ne 32 1
28 2XMM J061705.2+222129 XB* 06 17 05.26 +22 21 29.4           ~ 44 1
29 IC 443 SNR 06 18 02.7 +22 39 36           ~ 1108 1
30 HD 259440 HXB 06 32 59.2566624297 +05 48 01.162565528 9.17 9.58 9.12     B0pe 190 0
31 NAME Monoceros SNR SNR 06 38 43 +06 30.2           ~ 216 0
32 HD 261393 * 06 39 13.0934422731 +06 37 53.980834203   10.04 10.03     B5V 3 0
33 HD 49798 HXB 06 48 04.7000758397 -44 18 58.432035331 6.758 8.017 8.287 8.391 8.543 sdO6 285 0
34 HD 63666 HXB 07 47 23.5848135213 -53 19 56.823858254   7.60 7.60     B7IV/V 25 0
35 PSR J0821-4300 Psr 08 21 58.2 -43 00 22           ~ 114 2
36 NAME Pup A SNR 08 24 07 -42 59.8           ~ 523 1
37 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1123 2
38 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545           ~ 2072 1
39 NAME Vela Jr SN SNR 08 52.0 -46 20           ~ 407 2
40 2XMM J085201.4-461753 X 08 52 01.4 -46 17 53           ~ 39 1
41 V* GP Vel HXB 09 02 06.8610736194 -40 33 16.896402010 6.85 7.37 6.87 6.31 6.05 B0.5Ia 1376 0
42 SNR G038.7-01.3 SNR 09 06 40.50 +04 28 18.8           ~ 11 0
43 SN 1993J SN* 09 55 24.77476 +69 01 13.7026   10.8 12.0     SNIIb 1262 1
44 PSR J1016-58 Psr 10 16 21.266 -58 57 11.70           ~ 86 3
45 SNR G284.3-01.8 Rad 10 18.3 -59 00           ~ 101 2
46 3FHL J1018.8-5857 HXB 10 19 02.270 -58 56 29.87           ~ 94 0
47 CXOU J111148.6-603926 X 11 11 48.62 -60 39 26.2           ~ 2 0
48 SNR G291.0-00.1 SNR 11 11 54 -60 38.0           ~ 87 0
49 HD 102567 Be* 11 48 00.0214627917 -62 12 24.900348094 8.24 9.06 9.00 9.62   O/Bne 289 0
50 SNR G296.1-00.5 SNR 11 51 10 -62 34.0           ~ 47 0
51 SNR G295.5+09.7 SNR 12 09 40 -52 25.0           ~ 259 1
52 PSR J1210-5226 Psr 12 10 00.88 -52 26 28.4           ~ 206 1
53 HD 109857 Be* 12 39 14.57557 -75 22 14.1384 6.33         B8Vn 57 0
54 HD 110432 Be* 12 42 50.2655719413 -63 03 31.048323668 4.79 5.58 5.31     B0.5IVpe 271 0
55 * mu.02 Cru Be* 12 54 36.8837228156 -57 10 07.196143361 4.59 5.09 5.20 5.00 5.06 B5Vne 157 0
56 V* V850 Cen HXB 13 01 17.0966951298 -61 36 06.636402972   15.6       B2Vne 276 0
57 SN 2011dh SN* 13 30 05.10555 +47 10 10.9227           SNIIb 286 1
58 SNR G309.2-00.6 SNR 13 46.5 -62 54           ~ 59 0
59 [GV2003] N X 14 40 31.05 -62 38 16.9           ~ 6 0
60 SNR G315.0-02.3 SNR 14 43 00 -62 30.0           ~ 346 1
61 iPTF 13bvn SN* 15 00 00.152 +01 52 53.17           SNIb 107 0
62 NAME Lupus SN SNR 15 02 22.1 -42 05 49           ~ 1217 1
63 NAME Lupus Loop SNR 15 10.0 -40 00           ~ 60 0
64 HESS J1514-591 Rad 15 13 17.000 -59 04 54.00           ~ 379 3
65 PSR B1509-58 Psr 15 13 55.52 -59 08 08.8           ~ 798 1
66 Kes 25 SNR 15 53 00.000 -56 10 00.00           ~ 115 0
67 HD 141926 Be* 15 54 21.7677314365 -55 19 44.309668396 8.71 9.47 9.13 9.38   B2IIIn 59 0
68 PKS 1613-50 Rad 16 17 33.000 -51 02 00.00           ~ 457 3
69 2E 3623 X 16 17 36.30 -51 02 26.6           ~ 89 1
70 SNR G332.5-05.6 SNR 16 43.3 -54 30           ~ 24 0
71 HD 153919 HXB 17 03 56.7728262865 -37 50 38.912077679 6.06 6.78 6.51 6.08 5.90 O6Iafcp 760 1
72 SNR G343.1-02.3 SNR 17 08.0 -44 16           ~ 64 1
73 PSR B1706-44 Psr 17 09 42.62 -44 29 05.8           ~ 577 1
74 NAME Kepler SNR Rad 17 30 35.976 -21 28 56.23           ~ 716 4
75 HD 161103 Be* 17 44 45.7657852846 -27 13 44.482410725 8.44 9.23 9.13 9.12   B0.5III/IVe 73 0
76 IGR J17544-2619 HXB 17 54 25.2724584579 -26 19 52.578788584   14.71 12.94 12.10 10.38 O9Ib 165 0
77 PSR B1806-19.3 Psr 18 09 43.147 -19 17 38.10           ~ 71 1
78 SNR G011.1+00.1 SNR 18 09.8 -19 12           ~ 19 0
79 SNR G007.7-03.7 SNR 18 17 25 -24 04.0           ~ 40 0
80 V* V479 Sct HXB 18 26 15.0561532140 -14 50 54.249464136 12.02 12.23 11.27 11.04   ON6V((f))z 496 2
81 SNR G025.1-02.3 SNR 18 45 10 -08 00.0           ~ 11 0
82 2MASS J18511447-0000036 X 18 51 14.472 -00 00 03.64           ~ 9 0
83 4C -00.73 Rad 18 51 25 -00 08.0           ~ 84 1
84 PSR J1853-0004 Psr 18 53 23.02 -00 04 32.3           ~ 21 0
85 PSR B1853+01 Psr 18 56 10.65 +01 13 21.3           ~ 180 1
86 SNR G034.6-00.5 SNR 18 56 10.650 +01 13 21.30           ~ 831 2
87 XTE J1901+014 XB* 19 01 40.2 +01 26 31           ~ 49 1
88 SNR G039.7-02.0 SNR 19 12 20 +04 55.0           ~ 315 1
89 SNR G055.7+03.4 SNR 19 21.3 +21 44           ~ 34 0
90 PSR B1919+21 Psr 19 21 44.815 +21 53 02.25           ~ 347 0
91 PSR J1931+30 Psr 19 31 28 +30 35.0           ~ 9 0
92 SNR G065.2+05.7 SNR 19 33.0 +31 10           ~ 89 0
93 SNR G053.6-02.2 SNR 19 38.8 +17 14           ~ 137 0
94 SNR G065.7+01.2 SNR 19 52 13.70 +29 25 08.0           ~ 84 0
95 1WGA J1952.2+2925 X 19 52 17.0 +29 25 53           ~ 8 0
96 SNR G068.8+02.6 SNR 19 52 55 +32 54.2           ~ 328 1
97 PSR B1951+32 Psr 19 52 58.181 +32 52 40.98           ~ 550 2
98 HD 226868 HXB 19 58 21.6758193269 +35 12 05.782512305 9.38 9.72 8.91 8.42   O9.7Iabpvar 3947 0
99 SNR G082.2+05.3 SNR 20 19.0 +45 30           ~ 86 0
100 NAME gam Cyg SNR SNR 20 20 17.100 +40 26 09.00           ~ 200 2
101 PSR J2021+4026 Psr 20 21 30.496 +40 26 53.56           ~ 208 2
102 BD+47 3129 Em* 20 30 30.8457252623 +47 51 50.718662840 8.95 9.57 9.27     B0 32 0
103 SNR G089.0+04.7 SNR 20 45.0 +50 35           ~ 197 0
104 SNR G085.4+00.7 SNR 20 50.7 +45 22           ~ 27 0
105 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 826 0
106 SNR G093.2+06.7 SNR 20 52 25 +55 19.3           ~ 72 0
107 SNR G085.9-00.6 SNR 20 58.7 +44 53           ~ 26 0
108 BD+49 3718 HXB 22 01 38.2020869992 +50 10 04.633112055 8.95 9.47 9.31     Be 34 0
109 SNR G106.3+02.7 SNR 22 27.5 +60 50           ~ 40 1
110 PSR J2229+6114 Psr 22 29 05.262 +61 14 08.48           ~ 178 2
111 SN 2001ig SN* 22 57 30.69 -41 02 25.9     14.5     SNIIb 141 1
112 2E 4673 HXB 23 01 08.14 +58 52 44.5           ~ 588 1
113 SNR G109.1-01.0 SNR 23 01 35 +58 53.0           ~ 316 0
114 NAME Cas A SNR 23 23 24.000 +58 48 54.00           ~ 2437 1
115 TYC 4280-562-1 * 23 35 52.8676300804 +61 50 31.125502033   11.97 11.78     ~ 2 0
116 PSR B2334+61 Psr 23 37 05.779 +61 51 01.69           ~ 166 1
117 SNR G114.3+00.3 SNR 23 37 05.780 +61 51 01.69           ~ 109 1
118 CTB 1 SNR 23 59 13 +62 26.2           ~ 141 0

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2020.10.19-18:26:28

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