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arXiv · 1205.2182

On the origin of [Ne II] emission in young stars: mid-infrared and optical observations with the Very Large Telescope

C. Baldovin-Saavedra·M. Audard·A. Carmona·M. Guedel·K. Briggs·L. M. Rebull·S. L. Skinner·B. Ercolano
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Abstract

{Abridged version for ArXiv}. We provide direct constraints on the origin of the [Ne II] emission in 15 young stars using high-spatial and spectral resolution observations with VISIR at the VLT that allow us to study the kinematics of the emitting gas. In addition we compare the [Ne II] line with optical forbidden lines observed for three stars with UVES. The [Ne II] line was detected in 7 stars, among them the first confirmed detection of [Ne II] in a Herbig Be star, V892 Tau. In four cases, the large blueshifted lines indicate an origin in a jet. In two stars, the small shifts and asymmetric profiles indicate an origin in a photo-evaporative wind. CoKu Tau 1, seen close to edge-on, shows a spatially unresolved line centered at the stellar rest velocity, although cross-dispersion centroids move within 10 AU from one side of the star to the other as a function of wavelength. The line profile is symmetric with wings extending up to about +-80 km/s. The origin of the [Ne II] line could either be due to the bipolar jet or to the disk. For the stars with VLT-UVES observations, in several cases, the optical forbidden line profiles and shifts are very similar to the profile of the [Ne II] line, suggesting that the lines are emitted in the same region. A general trend observed with VISIR is a lower line flux when compared with the fluxes obtained with Spitzer. We found no correlation between the line full-width at half maximum and the line peak velocity. The [Ne II] line remains undetected in a large part of the sample, an indication that the emission detected with Spitzer in those stars is likely extended.

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C. Baldovin-Saavedra, M. Audard, A. Carmona, M. Guedel, K. Briggs, L. M. Rebull, S. L. Skinner, B. Ercolano. 2012-05-23. On the origin of [Ne II] emission in young stars: mid-infrared and optical observations with the Very Large Telescope. https://doi.org/10.1051/0004-6361%2F201118329

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