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20052026
most citedA survey of the high order multiplicity of nearby solar-type binary stars with Robo-AO

275 citations · 3.1k across the 84 of their papers we have counts for

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Showing astro-ph.SRShow all

24 papers · 1 filter

astro-ph.SR2022

An Adaptive Optics Census of Companions to Northern Stars Within 25 pc with Robo-AO

Maissa Salama, Carl Ziegler, Christoph Baranec +8

In order to assess the multiplicity statistics of stars across spectral types and populations in a volume-limited sample, we censused nearby stars for companions with Robo-AO. We r…

astro-ph.SR2021★ 19 cited

Large Adaptive Optics Survey for Substellar Objects (LASSO) Around Young, Nearby, Low-mass Stars with Robo-AO

Maissa Salama, James Ou, Christoph Baranec +16

We present results from the Large Adaptive optics Survey for Substellar Objects (LASSO), where the goal is to directly image new substellar companions (<70 M) at wide orbit…

astro-ph.SR2020★ 165 cited

When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147

Jason Lee Curtis, Marcel A. Agüeros, Sean P. Matt +17

Recent measurements of rotation periods () in the benchmark open clusters Praesepe (670 Myr), NGC 6811 (1 Gyr), and NGC 752 (1.4 Gyr) demonstrate that, after convergi…

astro-ph.SR2020★ 41 cited

Robo-AO M Dwarf Multiplicity Survey: Catalog

Claire Lamman, Christoph Baranec, Zachory K. Berta-Thompson +10

We analyze observations from Robo-AO's field M dwarf survey taken on the 2.1m Kitt Peak telescope and perform a multiplicity comparison with Gaia DR2. Through its laser-guided, aut…

astro-ph.SR2019★ 9 cited

Robo-AO Kepler Asteroseismic Survey. II. Do Stellar Companions Inhibit Stellar Oscillations?

Jessica Schonhut-Stasik, Daniel Huber, Christoph Baranec +7

The Kepler space telescope observed over 15,000 stars for asteroseismic studies. Of these, 75% of dwarfs (and 8% of giants) were found to show anomalous behavior: such as suppresse…

astro-ph.SR2019★ 14 cited

Investigating the origin of the spectral line profiles of the Hot Wolf-Rayet Star WR2

A. -N. Chené, N. St-Louis, A. F. J. Moffat +12

The hot WN star WR2 (HD6327) has been claimed to have many singular characteristics. To explain its unusually rounded and relatively weak emission line profiles, it has been propos…