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20112022
most citedMOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections

235 citations · 1.7k across the 36 of their papers we have counts for

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29 papers · 1 filter

astro-ph.SR2022★ 30 cited

The VLT-FLAMES Tarantula Survey: Observational evidence for two distinct populations of massive runaway stars in 30 Doradus

H. Sana, O. H. Ramírez-Agudelo, V. Hénault-Brunet +17

Two main scenarios have been proposed for origin of massive runaway stars -- dynamical ejection or release from a binary at the first core collapse -- but their relative contributi…

astro-ph.SR2022★ 7 cited

Distance and age of the massive stellar cluster Westerlund 1. II. The eclipsing binary W36

Danilo F. Rocha, Leonardo A. Almeida, Augusto Damineli +3

Westerlund 1 (Wd 1) is one of the most relevant star clusters in the Milky Way to study massive star formation, although it is still poorly known. Here, we used photometric and spe…

astro-ph.SR2022★ 19 cited

Distance and age of the massive stellar cluster Westerlund 1. I. Parallax method using Gaia-EDR3

Felipe Navarete, Augusto Damineli, Aura E. Ramirez +2

Westerlund 1 (Wd 1) is one of the most massive young star clusters in the Milky Way. Although relevant for star formation and evolution, its fundamental parameters are not yet very…

astro-ph.SR2022★ 11 cited

Rotation signature of TESS B-type stars. A comprehensive analysis

L. F. Barraza, R. L. Gomes, Y. S. Messias +11

Stellar rotation is a fundamental observable that drives different aspects of stellar and planetary evolution. In this work, we present an unprecedented manifold analysis of 160 B-…

astro-ph.SR2022

An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing

Kailash C. Sahu, Jay Anderson, Stefano Casertano +90

We report the first unambiguous detection and mass measurement of an isolated stellar-mass black hole (BH). We used the Hubble Space Telescope (HST) to carry out precise astrometry…

astro-ph.SR2021★ 9 cited

Probing the low-mass end of the companion mass function for O-type stars

M. Reggiani, A. Rainot, H. Sana +6

Almost all massive stars are part of a binary system. Given the wide range of separations at which these companions are found, several observational techniques have been adopted to…

astro-ph.SR2021★ 42 cited

The B-type Binaries Characterisation Programme I. Orbital solutions for the 30 Doradus population

J. I. Villaseñor, W. D. Taylor, C. J. Evans +6

We present results from the B-type Binaries Characterisation (BBC) programme, a multi-epoch spectroscopic study of 88 early B-type binary candidates in the 30 Doradus region of the…

astro-ph.SR2021★ 34 cited

Constraining the Overcontact Phase in Massive Binary Evolution I. Mixing in V382 Cyg, VFTS 352, and OGLE SMC-SC10 108086

Michael Abdul-Masih, Hugues Sana, Calum Hawcroft +10

As potential progenitors of several exotic phenomena including gravitational wave sources, magnetic stars, and Be stars, close massive binary systems probe a crucial area of the pa…

astro-ph.SR2021★ 7 cited

Search for magnetic accretion in SW Sextantis systems

I. J. Lima, C. V. Rodrigues, C. E. Ferreira Lopes +9

SW Sextantis systems are nova-like cataclysmic variables that have unusual spectroscopic properties, which are thought to be caused by an accretion geometry having part of the mass…

astro-ph.SR2020

A search for rotation periods in 1000 TESS objects of interest

Bruno L. Canto Martins, Roseane L. Gomes, Yuri S. Messias +8

The high quality light curves from the Transiting Exoplanet Survey Satellite (TESS) represent a unique laboratory for the study of stellar rotation, a fundamental observable drivin…

astro-ph.SR2020

The Carina High-Contrast Imaging Project for massive Stars (CHIPS) I. Methodology and proof of concept on QZ Car ( HD93206)

A. Rainot, M. Reggiani, H. Sana +13

Massive stars like company. However, low-mass companions have remained extremely difficult to detect at angular separations () smaller than 1" (~1000-3000 au considering typical…

astro-ph.SR2020★ 13 cited

Exploratory Spectroscopy of Magnetic Cataclysmic Variables Candidates and Other Variable Objects II

Alexandre S. Oliveira, Claudia V. Rodrigues, Murilo Martins +4

This is the second paper of a series presenting our search for magnetic Cataclysmic Variables (mCVs) among candidates selected mostly from the Catalina Real-Time Transient Survey (…

astro-ph.SR2019★ 67 cited

The Tarantula Massive Binary Monitoring: III. Atmosphere analysis of double-lined spectroscopic systems

L. Mahy, H. Sana, M. Abdul-Masih +17

Accurate stellar parameters of individual objects in binary systems are essential to constrain the effects of binarity on stellar evolution. These parameters serve as a prerequisit…

astro-ph.SR2019★ 49 cited

The Tarantula Massive Binary Monitoring. IV. Double-lined photometric binaries

L. Mahy, L. A. Almeida, H. Sana +10

A high fraction of massive stars are found to be binaries but only a few of them are reported as photometrically variable. By studying the populations of SB2 in the 30 Doradus regi…

astro-ph.SR2019★ 109 cited

Properties of OB star-black hole systems derived from detailed binary evolution models

N. Langer, C. Schürmann, K. Stoll +38

The recent gravitational wave measurements have demonstrated the existence of stellar mass black hole binaries. It is essential for our understanding of massive star evolution to i…

astro-ph.SR2019★ 43 cited

Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352

Michael Abdul-Masih, Hugues Sana, Jon Sundqvist +10

The massive O4.5 V + O5.5 V binary VFTS 352 in the Tarantula nebula is one of the shortest-period and most massive overcontact binaries known. Recent theoretical studies indicate t…

astro-ph.SR2019★ 15 cited

Orbital period variation of KIC 10544976: Applegate mechanism versus light travel time effect

Leonardo A. Almeida, Leandro de Almeida, Augusto Damineli +6

In recent years, several close post-common-envelope eclipsing binaries have been found to show cyclic eclipse timing variations (ETVs). This effect is usually interpreted either as…

astro-ph.SR2017★ 12 cited

HS 2231+2441: an HW Vir system composed by a low-mass white dwarf and a brown dwarf

Leonardo A. Almeida, Augusto Damineli, Cláudia V. Rodrigues +2

HW Vir systems are rare evolved eclipsing binaries composed by a hot compact star and a low-mass main-sequence star in a close orbit. These systems provide a direct way to measure…

astro-ph.SR2016★ 154 cited

The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries

L. A. Almeida, H. Sana, W. Taylor +24

Massive binaries (MBs) play a crucial role in the Universe. Knowing the distributions of their orbital parameters (OPs) is important for a wide range of topics, from stellar feedba…

astro-ph.SR2016★ 23 cited

Exploratory Spectroscopy of Magnetic Cataclysmic Variables Candidates and Other Variable Objects

A. S. Oliveira, C. V. Rodrigues, D. Cieslinski +5

The increasing number of synoptic surveys made by small robotic telescopes, such as the photometric Catalina Real-Time Transient Survey (CRTS), represents a unique opportunity for…

astro-ph.SR2015★ 74 cited

Discovery of the massive overcontact binary VFTS 352: Evidence for enhanced internal mixing

L. A. Almeida, H. Sana, S. E. de Mink +15

The contact phase expected to precede the coalescence of two massive stars is poorly characterized due to the paucity of observational constraints. Here we report on the discovery…

astro-ph.SR2014★ 19 cited

Candidate Gravitational Microlensing Events for Future Direct Lens Imaging

C. B. Henderson, H. Park, T. Sumi +76

The mass of the lenses giving rise to Galactic microlensing events can be constrained by measuring the relative lens-source proper motion and lens flux. The flux of the lens can be…

astro-ph.SR2014

MLS110213:022733+130617: A new eclipsing polar above the period gap

K. M. G. Silva, C. V. Rodrigues, A. S. Oliveira +4

We present new data that confirm MLS110213:022733+130617 as a new eclipsing polar. Some system properties were estimated.

astro-ph.SR2013★ 51 cited

Microlensing Discovery of a Population of Very Tight, Very Low-mass Binary Brown Dwarfs

J. -Y. Choi, C. Han, A. Udalski +121

Although many models have been proposed, the physical mechanisms responsible for the formation of low-mass brown dwarfs are poorly understood. The multiplicity properties and minim…