Circumstellar disks of the most vigorously accreting young stars.
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ABSTRACT:
SUBMITTER: Liu HB
PROVIDER: S-EPMC4788476 | biostudies-literature | 2016 Feb
REPOSITORIES: biostudies-literature
Publications
Circumstellar disks of the most vigorously accreting young stars.
Liu Hauyu Baobab HB Takami Michihiro M Kudo Tomoyuki T Hashimoto Jun J Dong Ruobing R Vorobyov Eduard I EI Pyo Tae-Soo TS Fukagawa Misato M Fukagawa Misato M Tamura Motohide M Henning Thomas T Dunham Michael M MM Karr Jennifer L JL Kusakabe Nobuhiko N Tsuribe Toru T
Science advances 20160205 2
Stars may not accumulate their mass steadily, as was previously thought, but in a series of violent events manifesting themselves as sharp stellar brightening. These events can be caused by fragmentation due to gravitational instabilities in massive gaseous disks surrounding young stars, followed by migration of dense gaseous clumps onto the star. Our high-resolution near-infrared imaging has verified the presence of the key associated features, large-scale arms and arcs surrounding four young s ...[more]
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