@inproceedings{03e314bd741145c1b88c2d3be24f1bfd,
title = "Spectral energy distributions of fragmenting protostellar disks",
abstract = "In this article we show that massive and hot fragments forming in protostellar disks can leave characteristic signatures in spectral energy distributions (SEDs) of young stellar objects. This occurs when the fragment evaporates dust in its atmosphere, which results in a sharp drop in opacity and subsequent rise in the surface temperature of the fragment. These hot fragments can produce local maxima in the SEDs at 5-10 μm.",
keywords = "planetary systems: protoplanetary disks, stars: formation",
author = "Olga Zakhozhay and Eduard Vorobiev",
year = "2014",
doi = "10.1017/S1743921313012982",
language = "English",
isbn = "9781107033825",
volume = "8",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
number = "S293",
pages = "278--280",
booktitle = "Formation, Detection, and Characterization of Extrasolar Habitable Planets",
edition = "S293",
}