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- W2045894791 abstract "The Eskimo Nebula (NGC 2392) is a double-shell planetary nebula (PN) known for the exceptionally large expansion velocity of its inner shell, ~90 km s-1, and the existence of a fast bipolar outflow with a line-of-sight expansion velocity approaching 200 km s-1. We have obtained XMM-Newton observations of the Eskimo and detected diffuse X-ray emission within its inner shell. The X-ray spectra suggest thin plasma emission with a temperature of ~2 106 K and an X-ray luminosity of erg s-1, where d is the distance in parsecs. The diffuse X-ray emission shows noticeably different spatial distributions between the 0.2–0.65 keV and 0.65–2.0 keV bands. High-resolution X-ray images of the Eskimo are needed to determine whether its diffuse X-ray emission originates from shocked fast wind or bipolar outflows." @default.
- W2045894791 created "2016-06-24" @default.
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- W2045894791 date "2005-01-26" @default.
- W2045894791 modified "2023-10-17" @default.
- W2045894791 title "<i>XMM-Newton</i> detection of hot gas in the Eskimo Nebula: Shocked stellar wind or collimated outflows?" @default.
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- W2045894791 doi "https://doi.org/10.1051/0004-6361:200400131" @default.
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