@article{0cccad5d0a0f4cb1af88c3f7a40ebb2f,
title = "On the Apparent Absence of Wolf-Rayet+Neutron Star Systems: The Curious Case of WR124",
abstract = "Among the different types of massive stars in advanced evolutionary stages is the enigmatic WN8h type. There are only a few Wolf-Rayet (WR) stars with this spectral type in our Galaxy. It has long been suggested that WN8h-type stars are the products of binary evolution that may harbor neutron stars (NS). One of the most intriguing WN8h stars is the runaway WR 124 surrounded by its magnificent nebula M1-67. We test the presence of an accreting NS companion in WR 124 using ∼100 ks long observations by the Chandra X-ray observatory. The hard X-ray emission from WR 124 with a luminosity of L X ∼ 1031 erg s-1 is marginally detected. We use the non-local thermodynamic equilibrium stellar atmosphere code PoWR to estimate the WR wind opacity to the X-rays. The wind of a WN8-type star is effectively opaque for X-rays, hence the low X-ray luminosity of WR 124 does not rule out the presence of an embedded compact object. We suggest that, in general, high-opacity WR winds could prevent X-ray detections of embedded NS, and be an explanation for the apparent lack of WR+NS systems.",
keywords = "ISM: jets and outflows, circumstellar matter, stars: Wolf-Rayet, stars: evolution, stars: massive, stars: neutron",
author = "Toal{\'a}, {J. A.} and Oskinova, {L. M.} and Hamann, {W. R.} and R. Ignace and Sander, {A. A.C.} and T. Shenar and H. Todt and Chu, {Y. H.} and Guerrero, {M. A.} and R. Hainich and Torrej{\'o}n, {J. M.}",
note = "Funding Information: The authors are indebted to the anonymous referee for a detailed revision of the manuscript and constructive suggestions. Support for this Letter was provided by the National Aeronautics and Space Administration through Chandra award No. G07-18014X issued by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the NASA contract NAS8-03060. J.A.T., M.A.G., and H.T. are funded by UNAM DGAPA PAPIIT project IA100318. L.M.O. acknowledges support by the DLR grant 50 OR 1508 and partial support by the Russian Government Program of Competitive Growth of Kazan Federal University. A.A.C.S. is supported by the Deutsche Forschungsgemeinschaft (DFG) under grant HA 1455/26 and would like to thank STFC for funding under grant No. ST/R000565/1. Y.-H.C. acknowledges support from the Ministry of Science and Technology of Taiwan. T.S. acknowledges support from the German Verbundforschung (DLR) grant 50 OR 1612. J.M.T. acknowledges support from ESP2017-85691-P. Publisher Copyright: {\textcopyright} 2018. The American Astronomical Society. All rights reserved..",
year = "2018",
month = dec,
day = "10",
doi = "10.3847/2041-8213/aaf39d",
language = "English (US)",
volume = "869",
journal = "Astrophysical Journal Letters",
issn = "2041-8205",
publisher = "IOP Publishing Ltd.",
number = "1",
}