2017ApJ...842..125Z


Query : 2017ApJ...842..125Z

2017ApJ...842..125Z - Astrophys. J., 842, 125-125 (2017/June-3)

Predicting the presence of companions for stripped-envelope supernovae: the case of the broad-lined Type Ic SN 2002ap.

ZAPARTAS E., DE MINK S.E., VAN DYK S.D., FOX O.D., SMITH N., BOSTROEM K.A., DE KOTER A., FILIPPENKO A.V., IZZARD R.G., KELLY P.L., NEIJSSEL C.J., RENZO M. and RYDER S.

Abstract (from CDS):

Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when these massive stars end their lives as core-collapse supernovae (SNe). We focus on stripped-envelope SNe, whose progenitors have lost their outer hydrogen and possibly helium layers before explosion. We use these results to interpret new Hubble Space Telescope observations of the site of the broad-lined Type Ic SN 2002ap, 14 years post-explosion. For a subsolar metallicity consistent with SN 2002ap, we expect a main-sequence (MS) companion present in about two thirds of all stripped-envelope SNe and a compact companion (likely a stripped helium star or a white dwarf/neutron star/black hole) in about 5% of cases. About a quarter of progenitors are single at explosion (originating from initially single stars, mergers, or disrupted systems). All of the latter scenarios require a massive progenitor, inconsistent with earlier studies of SN 2002ap. Our new, deeper upper limits exclude the presence of an MS companion star >8-10  M, ruling out about 40% of all stripped-envelope SN channels. The most likely scenario for SN 2002ap includes nonconservative binary interaction of a primary star initially 23 M. Although unlikely (<1% of the scenarios), we also discuss the possibility of an exotic reverse merger channel for broad-lined Type Ic events. Finally, we explore how our results depend on the metallicity and the model assumptions and discuss how additional searches for companions can constrain the physics that govern the evolution of SN progenitors.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): binaries: close - binaries: general - stars: evolution - stars: massive - supernovae: general - supernovae: individual: SN 2002ap - supernovae: individual: SN 2002ap

Simbad objects: 43

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Number of rows : 43
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 12559 1
2 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 5811 1
3 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 559 1
4 M 74 G 01 36 41.7451236624 +15 47 01.107512304 10.52 10.00 9.46 9.16   ~ 1710 1
5 PSR B0149-16 Psr 01 52 10.8520 -16 37 53.900           ~ 123 0
6 HD 12390 * 02 01 50.4088953792 +15 04 01.517124036   7.70 6.54     K0 12 0
7 HD 18391 s*y 02 59 48.7225501080 +57 39 47.673472140 10.56 8.83 6.89     G5Ia-Ib 103 0
8 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 6984 1
9 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 932 1
10 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 17264 1
11 M 1 SNR 05 34 30.9 +22 00 53           ~ 6156 1
12 SN 1987A SN* 05 35 28.020 -69 16 11.07           SNIIpec 4907 2
13 UCAC2 1803231 * 05 37 39.2300701008 -69 09 51.026810616 15.220 16.099 15.806 16.07 15.118 O9:Vnnne+ 27 0
14 PSR J0537-6910 Psr 05 37 46.66 -69 10 17.1           ~ 280 1
15 PSR J0538+2813 Psr 05 38 25.06 +28 17 11.0           ~ 196 2
16 RMC 136 Cl* 05 38 42.396 -69 06 03.36   5.81 5.40     ~ 2002 2
17 SNR G180.0-01.7 SNR 05 39 00.000 +27 50 00.00           ~ 249 2
18 HD 37424 * 05 39 44.4005541792 +27 46 51.188699784   9.05 8.99     B9 21 0
19 PSR B0628-28 Psr 06 30 49.3710 -28 34 42.200           ~ 294 0
20 NAME MONOCEROS NEB SNR 06 38 43 +06 30.2           ~ 247 0
21 SN 1997ef SN* 07 57 02.87 +49 33 41.3     16.5     SNIc-BL 270 1
22 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 543 0
23 PSR B0823+26 Psr 08 26 51.5068 +26 37 21.297           ~ 511 1
24 SN 2006jc SN* 09 17 20.78 +41 54 32.7     13.8     SNIbn 341 1
25 HD 83277 Pe* 09 36 31.8232900848 -27 57 45.149470020   8.57 8.29     F2VkA3mA3_lB? 43 0
26 SN 1993J SN* 09 55 24.77476 +69 01 13.7026   10.8 12.0     SNIIb 1410 1
27 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1202 1
28 SN 2004aw SN* 11 57 50.24 +25 15 55.1   18.06       SNIc 199 1
29 SN 2007ce SN* 12 10 17.96 +48 43 31.5     17.4     SNIc-BL 21 1
30 SN 2005cs SN* 13 29 53.37 +47 10 28.2   14.5       SNIIP 403 1
31 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 624 1
32 SN 2011dh SN* 13 30 05.10555 +47 10 10.9227           SNIIb 383 1
33 SN 2013cu SN* 14 33 58.97 +40 14 20.7           SNII: 85 1
34 iPTF 13bvn SN* 15 00 00.152 +01 52 53.17           SNIb 169 0
35 AJG 44 Psr 16 17 33.000 -51 02 00.00           ~ 505 3
36 2E 3623 X 16 17 36.30 -51 02 26.6           ~ 108 1
37 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1814 2
38 SNR G089.0+04.7 SNR 20 45.0 +50 35           ~ 223 0
39 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 909 0
40 SN 2001ig SN* 22 57 30.69 -41 02 25.9     14.5     SNIIb 172 1
41 SN 2003jd SN* 23 21 03.38 -04 53 45.5   16.34       SNIc-BL 139 1
42 NAME Cas A SNR 23 23 24.000 +58 48 54.00     14.30     ~ 2769 1
43 NAME Local Group GrG ~ ~           ~ 8311 0

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