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Cited article:

Synthesizing Spectra from 3D Radiation Hydrodynamic Models of Massive Stars Using Monte Carlo Radiation Transport

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Stochastic Low-frequency Variability in Three-dimensional Radiation Hydrodynamical Models of Massive Star Envelopes

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The Astrophysical Journal Letters 924 (1) L11 (2022)
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A new spectroscopic analysis of the massive O + O type binary HD 54662 AB

R H Barbá, C Sabín-Sanjulián, J I Arias, et al.
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Surface abundances of CNO in Galactic O-stars: a pilot study with FASTWIND

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Effective temperature of ionizing stars in extragalactic H iiregions – II. Nebular parameter relationships based on CALIFA data

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Angular Sizes and Effective Temperatures of O-type Stars from Optical Interferometry with the CHARA Array

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SPECTRAL CLASSIFICATION AND PROPERTIES OF THE O Vz STARS IN THE GALACTIC O-STAR SPECTROSCOPIC SURVEY (GOSSS)

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Accurate fundamental parameters and distance to a massive early-type eclipsing binary in the Danks 2 cluster

M. Kourniotis, A. Z. Bonanos, S. J. Williams, et al.
Astronomy & Astrophysics 582 A42 (2015)
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