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- W3102263490 abstract "Context. There exists an enigmatic population of massive stars around the Galactic center (GC) that were formed some Myr ago. A fraction of these stars has been found to orbit the supermassive black hole, Sgr A*, in a projected clockwise disk-like structure, which suggests that they were formed in a formerly existing dense disk around Sgr A*." @default.
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- W3102263490 date "2014-07-01" @default.
- W3102263490 modified "2023-09-25" @default.
- W3102263490 title "Properties of bow-shock sources at the Galactic center" @default.
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- W3102263490 doi "https://doi.org/10.1051/0004-6361/201423657" @default.
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