DM Ori: A Young Star Occulted by a Disturbance in its Protoplanetary Disk

In some planet formation theories, protoplanets grow gravitationally within a young star's protoplanetary disk, a signature of which may be a localized disturbance in the disk's radial and/or vertical structure. Using time-series photometric observations by the Kilodegree Extremely Little...

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Veröffentlicht in:	arXiv.org 2016-07
Hauptverfasser:	Rodriguez, Joseph E, Stassun, Keivan G, Cargile, Phillip, Shappee, Benjamin J, Siverd, Robert J, Pepper, Joshua, Lund, Michael B, Kochanek, Christopher S, James, David, Kuhn, Rudolf B, Beatty, Thomas G, Gaudi, B Scott, Weintraub, David A, Stanek, Krzysztof Z, Holoien, Thomas W S, Prieto, Jose L, Feldman, Daniel M, Espaillat, Catherine C
Format:	Artikel
Sprache:	eng
Schlagworte:	Dimming Photometry Physics - Solar and Stellar Astrophysics Planet formation Protoplanetary disks Protoplanets Sky surveys (astronomy) Spectral energy distribution Star & galaxy formation Supernovae
Online-Zugang:	Volltext
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