SIMBAD references

2014ApJ...786...63P - Astrophys. J., 786, 63 (2014/May-1)

[Fe II] emissions associated with the young interacting binary UY Aurigae.

PYO T.-S., HAYASHI M., BECK T.L., DAVIS C.J. and TAKAMI M.

Abstract (from CDS):

We present high-resolution 1.06-1.28 µm spectra toward the interacting binary UY Aur obtained with GEMINI/NIFS and the adaptive optics system Altair. We have detected [Fe II] λ1.257 µm and He I λ1.083 µm lines from both UY Aur A (the primary source) and UY Aur B (the secondary). In [Fe II] UY Aur A drives fast and widely opening outflows with an opening angle of ∼90° along a position angle of ∼40°, while UY Aur B is associated with a redshifted knot. The blueshifted and redshifted emissions show a complicated structure between the primary and secondary. The radial velocities of the [Fe II] emission features are similar for UY Aur A and B: ∼ -100 km/s for the blueshifted emission and ∼ +130 km/s for the redshifted component. The He I line profile observed toward UY Aur A comprises a central emission feature with deep absorptions at both blueshifted and redshifted velocities. These absorption features may be explained by stellar wind models. The He I line profile of UY Aur B shows only an emission feature.

Abstract Copyright:

Journal keyword(s): ISM: jets and outflows - stars: formation - stars: individual: UY Aurigae - stars: low-mass - stars: pre-main sequence - techniques: high angular resolution

Simbad objects: 11

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2020.10.22-06:28:50

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