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doi: 10.3847/1538-3881/aafe00 , 10.3847/1538-3881/aacb78 , 10.3847/1538-3881/acbe42 , 10.3847/1538-3881/ab4c94 , 10.3847/1538-3881/ab9b1e , 10.3847/1538-3881/adee23 , 10.3847/1538-3881/ac5330 , 10.48550/arxiv.1901.03655 , 10.48550/arxiv.2202.04056 , 10.48550/arxiv.1910.04143 , 10.48550/arxiv.1806.00027 , 10.48550/arxiv.2507.07233 , 10.48550/arxiv.2304.01861
doi: 10.3847/1538-3881/aafe00 , 10.3847/1538-3881/aacb78 , 10.3847/1538-3881/acbe42 , 10.3847/1538-3881/ab4c94 , 10.3847/1538-3881/ab9b1e , 10.3847/1538-3881/adee23 , 10.3847/1538-3881/ac5330 , 10.48550/arxiv.1901.03655 , 10.48550/arxiv.2202.04056 , 10.48550/arxiv.1910.04143 , 10.48550/arxiv.1806.00027 , 10.48550/arxiv.2507.07233 , 10.48550/arxiv.2304.01861
Abstract Spectroscopic orbits are determined for inner subsystems in nine stellar hierarchies (HIP 2863, 4974, 8353, 28796, 35261, 92929, 115272, 115552, and 117596). Their periods range from 2.5 to 312 days. For each system, estimates of masses, orbital inclination, and other parameters are given.
Visual binary stars, Astrophysics - Solar and Stellar Astrophysics, Astronomy, Astrophysics of Galaxies (astro-ph.GA), Spectroscopic binary stars, FOS: Physical sciences, QB1-991, Solar and Stellar Astrophysics, Multiple stars, Astrophysics - Astrophysics of Galaxies, Solar and Stellar Astrophysics (astro-ph.SR)
Visual binary stars, Astrophysics - Solar and Stellar Astrophysics, Astronomy, Astrophysics of Galaxies (astro-ph.GA), Spectroscopic binary stars, FOS: Physical sciences, QB1-991, Solar and Stellar Astrophysics, Multiple stars, Astrophysics - Astrophysics of Galaxies, Solar and Stellar Astrophysics (astro-ph.SR)
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 35 | |
popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |