Gemini-IFU spectroscopy of HH 111

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.

10 pages, 10 figures, accepted for publication in AJ

References in corpus (4)

• Recipes for stellar jets: results of combined optical/infrared diagnostics
• HST-Scale 3D simulations of MHD disc winds : A rotating two-component jet structure
• The Structure of the Inner HH 34 Jet from Optical Integral Field Spectroscopy
• Anatomy of HH 111 from CO observations : a bow shock driven molecular outflow