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2004BAVSR..53...18D - BAV Rundbrief, 53, 18-20 (2004/March-0)
KH15D und seine protoplanetare Scheibe.
DIEDERICH H.-G.
Abstract (from CDS):
KH15D (= V582 Mon) is a so called weak-lined T Tauri star (WTT). He was first observed in 1998 by Kearns and Herbst. The star shows minima about 18 days with a period of 48 days. Every year the minimum will take one day longer. There are indications that a protoplanatary disk causes the change of light. The elements of the mid-eclipse are: JD 2451626,86 + 48.34 * E.
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Simbad objects: 1
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