HV Tauri C - Herbig-Haro flow or stellar companion with strong forbidden emission lines?

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Stars: Pre-Main Sequence, Stars: Binaries: General, Stars: Individual: Hv Tau C

Scientific paper

We present new near- and mid-infrared photometry of the infrared source near HV Tau that was proposed as a Herbig-Haro object by Magazzu & Martin (\cite{magazzu}). We draw a different conclusion, namely that this object is a T Tauri star with strong forbidden emission lines as had been suggested originally. The presence of a Herbig-Haro flow in the vicinity of a weak-lined T Tauri star like HV Tau would have imposed a problem on models of T Tauri stars and their environment. With the reinstatement of the companion to HV Tau as a T Tauri star this problem disappears.

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