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.
Keywords
Cite
@article{arxiv.1501.03036,
title = {Gemini-IFU spectroscopy of HH 111},
author = {A. H. Cerqueira and M. J. Vasconcelos and A. C. Raga and J. Feitosa and H. Plana},
journal= {arXiv preprint arXiv:1501.03036},
year = {2015}
}
Comments
10 pages, 10 figures, accepted for publication in AJ