The Villafranca catalog of Galactic OB groups-II. From Gaia DR2 to EDR3 and ten new systems with O stars
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 the Galactic O-Star …
and photometric data from Gaia and spectral classifications from the Galactic O-Star …
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A
The evolution of massive stars is not completely understood. Several phenomena affect their
birth, life, and death, multiplicity being one of them. In this context, the OWN and MONOS …
birth, life, and death, multiplicity being one of them. In this context, the OWN and MONOS …
Non-synchronous rotations in massive binary systems-II. The case of HD 96264A
Context. The OWN Survey has detected several O-type stars with composite spectra whose
individual components show very different line broadening. Some of these stars have been …
individual components show very different line broadening. Some of these stars have been …
A new spectroscopic analysis of the massive O+ O type binary HD 54662 AB
ABSTRACT HD 54662 AB is one of the three O+ OB binaries known so far with orbital period
longer than 1000 d, offering the opportunity to test scenarios of massive star formation and …
longer than 1000 d, offering the opportunity to test scenarios of massive star formation and …
Rotational synchronisation of B-type binaries in 30 Doradus
DJ Lennon, PL Dufton, JI Villaseñor, N Langer… - arXiv preprint arXiv …, 2024 - arxiv.org
The spin evolution of stars in close binary systems can be strongly affected by tides. We
investigate the rotational synchronisation of the stellar components for 69 SB1 systems and …
investigate the rotational synchronisation of the stellar components for 69 SB1 systems and …
Asynchronous Rotation of a Massive Star in Close Binary Systems
SV Chernov - Astrophysics, 2022 - Springer
The problem of asynchronous rotation of massive stars in close binary systems is
investigated in this paper. A massive star with twice the sun's mass, a convective core, and …
investigated in this paper. A massive star with twice the sun's mass, a convective core, and …
[PDF][PDF] Open problems in high-mass stellar evolution
Massive stars can roughly be divided into two categories: the one that will become red
supergiants at (or shortly before) the end of their life, and those that will become Wolf-Rayet …
supergiants at (or shortly before) the end of their life, and those that will become Wolf-Rayet …
Determinación de parámetros astrofísicos fundamentales de estrellas masivas
CE Putkuri - 2019 - notablesdelaciencia.conicet.gov.ar
Las estrellas masivas son de vital importancia para el Universo, ie son los mayores
contribuyentes de la radiación UV en regiones de formación estelar y las responsables de …
contribuyentes de la radiación UV en regiones de formación estelar y las responsables de …
Properties of massive stars in Galactic binary systems
Within the OWN project, we use high resolution spectroscopic data of the massive binary
system HD54662 to measure accurate radial velocities and disentangle the spectra of the …
system HD54662 to measure accurate radial velocities and disentangle the spectra of the …