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- W2055046725 abstract "The supermassive black hole at the Galactic center is surrounded by a parsec-scale star disk, with about a hundred massive young stars that move in approximately circular Keplerian orbits. Another group of roughly 20 young stars (S-stars) follow eccentric, randomly oriented orbits well inside the disk stars. A model is proposed to explain the S-stars. Accordingly, the stars formed originally in the parsec-scale disk through gravitational fragmentation of gas. The newly formed S-stars then migrated inward via the gravitational torques exerted by a Lin-Shu-type spiral density wave on the stars at an inner Lindblad resonance." @default.
- W2055046725 created "2016-06-24" @default.
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- W2055046725 date "2009-08-11" @default.
- W2055046725 modified "2023-09-25" @default.
- W2055046725 title "ORIGIN OF THE GALACTIC CENTER S-STARS" @default.
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- W2055046725 doi "https://doi.org/10.1088/0004-637x/702/1/l1" @default.
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