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Articles citing this article

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Cited article:

Exciting Stellar Eccentricity in Gaia BH3 via a Hidden Black Hole Binary

Qingru 清茹 Hu 胡, Bin 彬 Liu 刘 and Wei 伟 Zhu 祝
The Astrophysical Journal Letters 994 (1) L18 (2025)
https://doi.org/10.3847/2041-8213/ae19e1

ESPRESSO Observations of Gaia BH1: High-precision Orbital Constraints and no Evidence for an Inner Binary

Pranav Nagarajan, Kareem El-Badry, Amaury H. M. J. Triaud, Thomas A. Baycroft, David Latham, Allyson Bieryla, Lars A. Buchhave, Hans-Walter Rix, Eliot Quataert, Andrew Howard, Howard Isaacson and Melissa J. Hobson
Publications of the Astronomical Society of the Pacific 136 (1) 014202 (2024)
https://doi.org/10.1088/1538-3873/ad1ba7

Constraining the Binarity of Black Hole Candidates: A Proof-of-concept Study of Gaia BH1 and Gaia BH2

Toshinori 利憲 Hayashi 林, Yasushi 靖 Suto 須藤 and Alessandro A. 虎似 Trani 三努郎
The Astrophysical Journal 958 (1) 26 (2023)
https://doi.org/10.3847/1538-4357/acf4f6

Theoretical analysis on pulsar timing of a millisecond pulsar around a binary black hole

Xiao-Jun Wu, Ye-Fei Yuan, Rajiv Kumar and Yan Luo
Monthly Notices of the Royal Astronomical Society 510 (1) 708 (2021)
https://doi.org/10.1093/mnras/stab3567

Unveiling the Architecture of a Pulsar–Binary Black Hole Triple System with Pulsar Arrival Time Analysis

Toshinori Hayashi (林 利憲) and Yasushi Suto (須藤 靖)
The Astrophysical Journal 907 (1) 48 (2021)
https://doi.org/10.3847/1538-4357/abcec6

Radial-velocity Variation of a Tertiary Star Orbiting a Binary Black Hole in Coplanar and Noncoplanar Triples: Short- and Long-term Anomalous Behavior

Toshinori 利憲 Hayashi 林 and Yasushi 靖 Suto 須藤
The Astrophysical Journal 897 (1) 29 (2020)
https://doi.org/10.3847/1538-4357/ab97ad

A Strategy to Search for an Inner Binary Black Hole from the Motion of the Tertiary Star

Toshinori 利憲 Hayashi 林, Shijie 士杰 Wang 汪 and Yasushi 藤靖 Suto 須
The Astrophysical Journal 890 (2) 112 (2020)
https://doi.org/10.3847/1538-4357/ab6de6

The discovery of a planetary candidate around the evolved low-massKeplergiant star HD 175370

M. Hrudková, A. Hatzes, R. Karjalainen, et al.
Monthly Notices of the Royal Astronomical Society 464 (1) 1018 (2017)
https://doi.org/10.1093/mnras/stw2379

Detectability of quasi-circular co-orbital planets. Application to the radial velocity technique

Adrien Leleu, Philippe Robutel and Alexandre C. M. Correia
Astronomy & Astrophysics 581 A128 (2015)
https://doi.org/10.1051/0004-6361/201526175

NEXT GENERATION OF TELESCOPES OR DYNAMICS REQUIRED TO DETERMINE IF EXO-MOONS HAVE PROGRADE OR RETROGRADE ORBITS

Karen M. Lewis and Yuka Fujii
The Astrophysical Journal 791 (2) L26 (2014)
https://doi.org/10.1088/2041-8205/791/2/L26

Precession due to a close binary system: an alternative explanation for ν-Octantis?

M. H. M. Morais and A. C. M. Correia
Monthly Notices of the Royal Astronomical Society 419 (4) 3447 (2012)
https://doi.org/10.1111/j.1365-2966.2011.19986.x

Spectroscopic orbits for K giants β Reticuli and ν Octantis: what is causing a low-amplitude radial velocity resonant perturbation in ν Oct?

D. J. Ramm, D. Pourbaix, J. B. Hearnshaw and S. Komonjinda
Monthly Notices of the Royal Astronomical Society 394 (3) 1695 (2009)
https://doi.org/10.1111/j.1365-2966.2009.14459.x