Speckle observations and orbits of multiple stars
arXiv:1908.11445 · doi:10.3847/1538-3881/ab4137
Abstract
We report results of speckle-interferometric monitoring of visual hierarchical systems using the newly commissioned instrument NESSI at the 3.5-m WIYN telescope. During one year, 390 measurements of 129 resolved subsystems were made, while some targets were unresolved. Using our astrometry and archival data, we computed 36 orbits (27 for the first time). Spectro-interferometric orbits of seven pairs are determined by combining positional measurements with radial velocities measured, mostly, with the Center for Astrophysics digital speedometers. For the hierarchical systems HIP 65026 (periods 49 and 1.23 years) and HIP 85209 (periods 34 and 1.23 years) we determined both the inner and the outer orbits using astrometry and radial velocities and measured the mutual orbit inclinations of 11.3+-1.0 deg and 12.0+-3.0 deg, respectively. Four bright stars are resolved for the first time; two of those are triple systems. Several visual subsystems announced in the literature are shown to be spurious. We note that subsystems in compact hierarchies with outer separations less than 100 au tend to have less eccentric orbits compared to wider hierarchies.
Accepted by The Astronomical Journal. 16 pages, 15 Figures, 8 Tables
References in corpus (12)
- Gaia Data Release 2. Summary of the contents and survey properties
- The Hipparcos-Gaia Catalog of Accelerations
- Planets Around Low-Mass Stars (PALMS). IV. The Outer Architecture of M Dwarf Planetary Systems
- Ten years of speckle interferometry at SOAR
- The Updated Multiple Star Catalog
- Orbit alignment in triple stars
- Speckle interferometry at SOAR in 2016 and 2017
- Dancing twins: stellar hierarchies that formed sequentially?
- Observations of Binary Stars with the Differential Speckle Survey Instrument. V. Toward an Empirical Metal-Poor Mass-Luminosity Relation
- Spectroscopic orbits of nearby stars
- Observations of Binary Stars with the Differential Speckle Survey Instrument. VIII. Measures of Metal-Poor Stars and Triple Stars from 2015 to 2018
- The unusual quadruple system HD 91962 with a "planetary" architecture
Cited by in corpus (10)
- The 10 parsec sample in the Gaia era
- A naked-eye triple system with a nonaccreting black hole in the inner binary
- The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy
- Orbital Architectures of Planet-Hosting Binaries II. Low Mutual Inclinations Between Planetary and Stellar Orbits
- Comparison of Gaia and Hipparcos parallaxes of close visual binary stars and the impact on determinations of their masses
- Speckle Interferometry of Nearby Multiple Stars: 2007-2019 Positional Measurements and Orbits of Eight Objects
- Detecting New Visual Binaries in Gaia DR3 with Gaia and 2MASS Photometry I. New Candidate Binaries Within 200 pc of the Sun
- Light-time effect detected in fourteen eclipsing binaries
- Orbital parallax of binary systems compared to GAIA DR3 and the parallax zero-point offset at bright magnitudes
- Vintage NPOI: New and Updated Angular Diameters for 145 Stars