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• W3104011605 abstract "We report VIMOS integral field spectroscopy of the N159F nebula surrounding LMC X-1. Our observations reveal a rich, extended system of emission-line filaments lining the boundary of a large conical cavity identified in Spitzer mid-IR imaging. We find that X-ray photoionization cannot be solely responsible for the observed ionization structure of N159F. We propose that the extended filamentary emission is produced primarily by ionization from a shock driven by a presently unobserved jet from LMC X-1. We infer a shock velocity of vs ≈ 90 km s-1 and conclude that the jet responsible for the bow shock is presently undetected because it has switched off, rather than because it has a low surface brightness. This interpretation is consistent with the present soft X-ray spectral state of LMC X-1 and suggests the jet is intermittent." @default.
• W3104011605 created "2020-11-23" @default.
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• W3104011605 date "2007-09-12" @default.
• W3104011605 modified "2023-09-23" @default.
• W3104011605 title "Spectacular Trailing Streamers near LMC X-1: The First Evidence of a Jet?" @default.
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• W3104011605 doi "https://doi.org/10.1086/522517" @default.
• W3104011605 hasPublicationYear "2007" @default.
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