activity
20202026
most citedIdentifying quiescent compact objects in massive Galactic single-lined spectroscopic binaries

81 citations · 285 across the 17 of their papers we have counts for

collaborators

17 papers

physics.gen-ph2026

Multiplicity of Massive Stars at Low Metallicity: Early Results from the BLOeM Campaign

T. Shenar, J. Bodensteiner, M. Abdul-Masih +73

Massive stars at low metallicity (Z) play a central role in shaping the high-redshift Universe, yet their multiplicity remains poorly constrained. The Binarity at Low Metallicity (…

astro-ph.SR2026

The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812

K. Deshmukh, H. Sana, O. Verhamme +9

Massive O-type stars () with an X-ray quiet black hole (BH) companion represent a crucial stage in massive binary evolution leading to binary BH mergers. The p…

astro-ph.SR2025

HOney-BeeS II. Be-X-ray binaries as testbeds for spectroscopic studies of Be stars

S. Janssens, H. Sana, T. Shenar +2

The majority of massive classical Be stars are thought to be binary interactions products. Their rapid rotation and often strong, variable, and emission-line dominated spectrum, ma…

astro-ph.SR2025★ 22 cited

A high fraction of close massive binary stars at low metallicity

H. Sana, T. Shenar, J. Bodensteiner +74

At high metallicity, a majority of massive stars have at least one close stellar companion. The evolution of such binaries is subject to strong interaction processes, heavily impac…

astro-ph.SR2025★ 1 cited

Two unseen massive white dwarf candidates in close binaries

Yuta Shiraishi, Kenta Hotokezaka, Kento Masuda +10

We report the discovery of two binary systems, each consisting of a slightly bloated G-type main-sequence star and an unseen companion, identified through photometric data from TES…

astro-ph.SR2025★ 4 cited

Binarity at LOw Metallicity (BLOeM): Bayesian inference of natal kicks from inert black hole binaries

R. Willcox, P. Marchant, A. Vigna-Gómez +15

Context. The emerging population of inert black hole binaries (BHBs) provides a unique opportunity to constrain black hole (BH) formation physics. These systems are composed of a s…

astro-ph.SR2025★ 17 cited

Binarity at Low Metallicity (BLOeM) -- Multiplicity properties of Oe and Be stars

J. Bodensteiner, T. Shenar, H. Sana +40

Rapidly rotating classical OBe stars have been proposed as the products of binary interactions, and the fraction of Be stars with compact companions implies that at least some are.…

astro-ph.SR2024★ 37 cited

Binarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC

T. Shenar, J. Bodensteiner, H. Sana +74

Surveys in the Milky Way and Large Magellanic Cloud revealed that the majority of massive stars will interact with companions during their lives. However, knowledge of the binary p…

astro-ph.SR2023★ 25 cited

MWC 656 is unlikely to contain a black hole

S. Janssens, T. Shenar, N. Degenaar +4

Context. MWC 656 was reported as the first known Be star with a black-hole (BH) companion in a 60 d period. The mass of the proposed BH companion is estimated to be between 4 - 7 M…

astro-ph.SR2022★ 8 cited

Detection of single-degenerate massive binaries with Gaia: The impact of blue supergiants, triples, mass precision, and high-precision parallax requirements

S. Janssens, T. Shenar, H. Sana +1

Hundreds of black holes with massive main-sequence companions (OB+BHs) might be identified from Gaia astrometry with the Astrometric Mass-Ratio Function (AMRF). We investigate the…

astro-ph.SR2022

The Nature of Unseen Companions in Massive Single-Line Spectroscopic Binaries

Hugues Sana, Michael Abdul-Masih, Gareth Banyard +14

Massive stars are predominantly found in binaries and higher order multiples. While the period and eccentricity distributions of OB stars are now well established across different…

astro-ph.SR2022★ 81 cited

Identifying quiescent compact objects in massive Galactic single-lined spectroscopic binaries

L. Mahy, H. Sana, T. Shenar +13

Aims. To search for these rare objects, we study 32 Galactic O-type stars that were reported as SB1s in the literature. In our sample we include Cyg X-1, which is known to host an…

astro-ph.SR2022★ 24 cited

Planet Hunters TESS IV: A massive, compact hierarchical triple star system TIC 470710327

Nora L. Eisner, Cole Johnston, Silvia Toonen +37

We report the discovery and analysis of a massive, compact, hierarchical triple system (TIC 470710327) initially identified by citizen scientists in data obtained by NASA's Transit…

astro-ph.SR2021★ 42 cited

Uncovering astrometric black hole binaries with massive main-sequence companions with Gaia

S. Janssens, T. Shenar, H. Sana +6

The hunt for compact objects is on. Rarely seen massive binaries with a compact object are a crucial phase in the evolution towards compact object mergers. In Gaia data release 3 (…

astro-ph.SR2021★ 4 cited

LBV phenomenon and binarity: The environment of HR Car

A. Mehner, S. Janssens, C. Agliozzo +7

Luminous blue variable stars (LBVs) are of great interest in massive-star evolution as they experience very high mass-loss episodes within short periods of time. HR Car is a famous…

astro-ph.SR2021★ 10 cited

A binary with a ~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821

Simon J Murphy, Tanda Li, Sanjay Sekaran +8

We study the Scuti -- red giant binary KIC9773821, the first double-pulsator binary of its kind. It was observed by \textit{Kepler} during its four-year mission. Our aims are t…

astro-ph.SR2020★ 10 cited

BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary

Soetkin Janssens, Tomer Shenar, Laurent Mahy +3

BAT99 126 is a multiple system in the Large Magellanic Cloud containing a Wolf-Rayet (WR) star, which has a reported spectroscopic (orbital) period of 25.5 days and a photometric (…