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20052026
most citedThe VLT-FLAMES Tarantula Survey VIII. Multiplicity properties of the O-type star population

530 citations · 5.8k across the 95 of their papers we have counts for

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Showing 2021Show all

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astro-ph.GA2021★ 15 cited

Escape from the Bermuda cluster: orphanization by multiple stellar ejections

J. Maíz Apellániz, M. Pantaleoni González, R. H. Barbá +1

CONTEXT. Dynamical interactions in young stellar clusters can eject massive stars early in their lives and significantly alter their mass functions. If all of the most massive star…

astro-ph.IM2021★ 57 cited

An estimation of the Gaia EDR3 parallax bias from stellar clusters and Magellanic Clouds data

J. Maíz Apellániz

CONTEXT. The Gaia EDR3 parallaxes constitute the most detailed and accurate dataset that can be currently used to determine stellar distances in the solar neighborhood. Nevertheles…

astro-ph.GA2021★ 44 cited

The Villafranca catalog of Galactic OB groups. II. From Gaia DR2 to EDR3 and ten new systems with O stars

J. Maíz Apellániz, R. H. Barbá, R. Fernández Aranda +4

CONTEXT. This is the second paper of a series on Galactic OB groups that uses astrometric and photometric data from Gaia and spectral classifications from GOSSS and LiLiMaRlin. The…

astro-ph.SR2021★ 14 cited

Hubble spectroscopy of LB-1: comparison with B+black-hole and Be+stripped-star models

D. J. Lennon, J. Maíz Apellániz, A. Irrgang +10

LB-1 has variously been proposed as either an X-ray dim B-type star plus black hole (B+BH) binary, or a Be star plus an inflated stripped star (Be+Bstr) binary. The Space Telescope…

astro-ph.SR2021★ 28 cited

The Tarantula Massive Binary Monitoring V. R 144: a wind-eclipsing binary with a total mass > 140 Msun

T. Shenar, H. Sana, P. Marchant +21

R 144 is the visually brightest WR star in the Large Magellanic Cloud (LMC). R 144 was reported to be a binary, making it potentially the most massive binary thus observed. We perf…