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• W3104201511 abstract "We present new optical observations of the HH 111 Herbig-Haro jet using the Gemini Multi Object Spectrograph in its Integral Field Unit mode. Eight fields of 5 x 3.5 have been positioned along and across the HH 111 jet, covering the spatial region from knot E to L in HH 111 (namely, knots E, F, G, H, J, K and L). We present images and velocity channel maps for the [O I] 6300+6360, Halpha, [N II] 6548+6583 and [S II] 6716+6730 lines, as well as for the [S II]6716/6730 line ratio. We find that the HH 111 jet has an inner region with lower excitation and higher radial velocity, surrounded by a broader region of higher excitation and lower radial velocity. Also, we find higher electron densities at lower radial velocities. These results imply that the HH 111 jet has a fast, axial region with lower velocity shocks surrounded by a lower velocity sheath with higher velocity shocks." @default.
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• W3104201511 date "2015-02-09" @default.
• W3104201511 modified "2023-09-24" @default.
• W3104201511 title "GEMINI-IFU SPECTROSCOPY OF HH 111" @default.
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• W3104201511 doi "https://doi.org/10.1088/0004-6256/149/3/98" @default.
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