Sylvana Yelda, Ph.D.
Affiliations: | 2012 | Astronomy 0099 | University of California, Los Angeles, Los Angeles, CA |
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"Sylvana Yelda"Mean distance: 15.22
Cross-listing: Astronomy Tree
Parents
Sign in to add mentor| Andrea Ghez | grad student | 2012 | UCLA | |
| (Constraining the Recent Star Formation History of the Galactic Center with High Precision Astrometry.) | ||||
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Publications
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| Witzel G, Sitarski BN, Ghez AM, et al. (2017) The Post-periapsis Evolution of Galactic Center Source G1: The Second Case of a Resolved Tidal Interaction with a Supermassive Black Hole The Astrophysical Journal. 847: 80 |
| Boehle A, Ghez AM, Schödel R, et al. (2016) AN IMPROVED DISTANCE and MASS ESTIMATE for SGR A∗ from A MULTISTAR ORBIT ANALYSIS Astrophysical Journal. 830 |
| Chappell SN, Ghez AM, Do T, et al. (2016) The late-type stellar density profile in the Galactic Center: A statistical approach Proceedings of the International Astronomical Union. 11: 235-236 |
| Støstad M, Do T, Murray N, et al. (2015) MAPPING the OUTER EDGE of the YOUNG STELLAR CLUSTER in the GALACTIC CENTER Astrophysical Journal. 808 |
| Schöck M, Do T, Ellerbroek BL, et al. (2014) Thirty Meter Telescope astrometry error budget Proceedings of Spie - the International Society For Optical Engineering. 9148 |
| Witzel G, Ghez AM, Morris MR, et al. (2014) Detection of Galactic Center source G2 at 3.8 μm during periapse passage Astrophysical Journal Letters. 796 |
| Schödel R, Feldmeier A, Neumayer N, et al. (2014) The nuclear cluster of the Milky Way: our primary testbed for the interaction of a dense star cluster with a massive black hole Classical and Quantum Gravity. 31: 244007 |
| Yelda S, Ghez AM, Lu JR, et al. (2014) Properties of the remnant clockwise disk of young stars in the galactic center Astrophysical Journal. 783 |
| Meyer L, Ghez AM, Witzel G, et al. (2014) The Keplerian orbit of G2 Proceedings of the International Astronomical Union. 9: 264-268 |
| Lu JR, Ghez AM, Morris MR, et al. (2014) Young stars in the Galactic center Proceedings of the International Astronomical Union. 9: 211-219 |