Accretion and outflow activity on the late phases of pre-main-sequence evolution: The case of RZ Piscium

RZPsc is an isolated high-latitude post-T Tauri star that demonstrates a UX Ori-type photometric activity. The star shows very weak spectroscopic signatures of accretion, but at the same time possesses the unusual footprints of the wind in NaiDlines. In the present work we investigate new spectrosco...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2017-03, Vol.599, p.A60
Hauptverfasser:	Potravnov, I S, Mkrtichian, D E, Grinin, V P, Ilyin, I V, Shakhovskoy, D N
Format:	Artikel
Sprache:	eng
Schlagworte:	Absorption Accretion Intervals Photometry Signatures Sodium Spectroscopy Stars
Online-Zugang:	Volltext
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