Concerning the occurrence of bow shocks around high-mass X-ray binaries.
作者： M. Prisegen
DOI: 10.1051/0004-6361/201832682
关键词:
摘要: We investigate the occurrence of stellar bow shocks around high-mass X-ray binaries (HMXBs) in Galaxy. seek to conduct a survey HMXBs mid-infrared search for presence these objects. Telescopes operating mid-infrared, such as Spitzer Space Telescope or Wide-field Infrared Survey Explorer (WISE), are potent tools searching shocks. used available archival data from telescopes shock candidates confirmed and candidate detected extended structures several surveyed HMXBs. Two structures, associated with Vela X-1 4U 1907+09, genuine that have been studied previously. However, there no new unambiguous among rest The paucity suggests majority systems still reside within hot, low-density bubbles their parent star clusters associations. This also implies dynamical ejection massive is apparently less efficient than ejections caused by supernova explosions inside binary.
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