Circumstellar disks of the most vigorously accreting young stars

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...

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Detalles Bibliográficos
Autores principales: Liu, Hauyu Baobab, Takami, Michihiro, Kudo, Tomoyuki, Hashimoto, Jun, Dong, Ruobing, Vorobyov, Eduard I., Pyo, Tae-Soo, Fukagawa, Misato, Tamura, Motohide, Henning, Thomas, Dunham, Michael M., Karr, Jennifer L., Kusakabe, Nobuhiko, Tsuribe, Toru
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2016
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4788476/
https://www.ncbi.nlm.nih.gov/pubmed/26989772
http://dx.doi.org/10.1126/sciadv.1500875

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4788476/
https://www.ncbi.nlm.nih.gov/pubmed/26989772
http://dx.doi.org/10.1126/sciadv.1500875

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