248 research outputs found
The 1996-1997 Fading of V651 Mon, the Binary Central Star of the Planetary Nebula NGC 2346
V651 Mon is the binary central star of the bipolar planetary nebula NGC 2346.
The star showed the second-ever deep fading in 1996-1997, which was presumably
caused by obscuration by a dust cloud in the planetary nebula, as was proposed
to explain the 1981-1985 event. The entire duration of the 1996-1997 event was
\~400 d, remarkably shorter than the 1981-1985 event, suggesting that the
obscuring body was smaller or had a larger tangential velocity. The most
remarkable feature in this event was the presence of a sharply defined
transient clearing (brightening). From the time-scale of the variation, we
propose an upper limit of the projected scale of several times ~10^11 cm of the
structure responsible for the brightening. This observation provides the first
evidence for a sharply defined, small lucent structure within the obscuring
body around the central star of NGC 2346Comment: 4 pages, 3 figures (using a non-standard style file
Temporal Variation of Cross-Shore Bottom Profile along an Observational Pier at Joetsu-Ogata Coast
Source: ICHE Conference Archive - https://mdi-de.baw.de/icheArchiv
Numerical Investigation on Effects of a Diversion Channel along a Meandering River Based on a 2D Model
Source: ICHE Conference Archive - https://mdi-de.baw.de/icheArchiv
Numerical Simulation on Prediction of Debris-Flow Hydrograph of Heterogeneous Bed Material and Sediment Transport in a Mountainous River
Debris-Flow Deposition and Erosion Processes of the Sediment Deposit Upstream of a Check Dam
Source: ICHE Conference Archive - https://mdi-de.baw.de/icheArchiv
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