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• W2013552456 abstract "New subarcsecond far-UV observations of T Tau with Hubble Space Telescope STIS show spatially resolved structures in the 2'' × 2'' area around the star. The structures are apparent in multiline emission of fluorescent H2 pumped by Lyα. One emission structure follows the cavity walls observed around T Tau N in scattered light in the optical. A temperature of ≥1000 K is required to have a high enough population in the H2 to produce the observed fluorescent lines; in the cool environment of the T Tau system, shock heating is required to achieve this temperature at distances of a few tens of AU. Fluorescent H2 along the cavity wall represents the best evidence to date for the action of low-density, wide opening angle outflows driving cavities into the molecular medium at scales ≤100 AU. A southern region of emission consists of two arcs, with shape and orientation similar to the arcs of H2 2.12 μm and forbidden-line emission crossing the outflow associated with the embedded system T Tau S. This region is located near the centroid of forbidden-line emission at the blueshifted lobe of the north-south outflow." @default.
• W2013552456 created "2016-06-24" @default.
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• W2013552456 date "2003-07-01" @default.
• W2013552456 modified "2023-10-01" @default.
• W2013552456 title "The Spatial Distribution of Fluorescent H₂Emission near T Tauri" @default.
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• W2013552456 doi "https://doi.org/10.1086/374885" @default.
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