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- W2023649858 abstract "With the Hubble Space Telescope's Wide Field Planetary Camera 2 we have obtained a deep, Hα image of the relatively young ejection-type nebula M1-67 around the runaway Population I Wolf-Rayet star WR 124 (WN 8). This image shows a wealth of complex detail, some of which have never been seen before in such a nebula. In particular, large arcs of nebulosity extend around the central star yet with no overall global shell structure to the nebula and no clear bipolar signature as claimed by Sirianni et al. In addition, numerous bright, mostly unresolved knots of emission, each ≲10-4 M☉, occur in the inner part of the nebula, often surrounded by what appear to be their own local wind diffuse bubbles. Is this the first direct evidence of spatially resolved hot clumps being ejected from a hot central star?" @default.
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- W2023649858 date "1998-10-20" @default.
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- W2023649858 title "[ITAL]HST[/ITAL] WFPC2/Hα Imagery of the Nebula M1-67: A Clumpy LBV Wind Imprinting Itself on the Nebular Structure?" @default.
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- W2023649858 doi "https://doi.org/10.1086/311647" @default.
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