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20002023
most citedThe pre- versus post-main sequence evolutionary phase of B[e] stars: Constraints from 13CO band emission

70 citations · 238 across the 24 of their papers we have counts for

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astro-ph.SR20235 cited

Unveiling the evolutionary state of three B supergiant stars: PU Gem, CMa and CMa

Julieta P. Sánchez Arias, Péter Németh, Elisson S. G. de Almeida +3

We aim to combine asteroseismology, spectroscopy, and evolutionary models to establish a comprehensive picture of the evolution of Galactic blue supergiant stars (BSG). To start su…

astro-ph.SR2023

BCD spectrophotometry for massive stars in transition phases

Y. J. Aidelman, M. Borges Fernandes, L. S. Cidale +7

Context. Stars in transition phases, like those showing the B[e] phenomenon and luminous blue variables (LBVs), undergo strong, often irregular mass ejection events. The prediction…

astro-ph.SR2023

New Insight into the FS CMa System MWC 645 from Near-Infrared and Optical Spectroscopy

Andrea F. Torres, María L. Arias, Michaela Kraus +2

The B[e] phenomenon is manifested by a heterogeneous group of stars surrounded by gaseous and dusty circumstellar envelopes with similar physical conditions. Among these stars, the…

astro-ph.SR2023

Dense Molecular Environments of B[e] Supergiants and Yellow Hypergiants

Michaela Kraus, Michalis Kourniotis, Maria Laura Arias +2

Massive stars expel large amounts of mass during their late evolutionary phases. We aim to unveil the physical conditions within the warm molecular environments of B[e] supergiants…

astro-ph.SR20231 cited

Large-Scale Ejecta of Z CMa -- Proper Motion Study and New Features Discovered

Tiina Liimets, Michaela Kraus, Lydia Cidale +2

Z Canis Majoris is a fascinating early-type binary with a Herbig Be primary and a FU Orionis-type secondary. Both of the stars exhibit sub-arcsecond jet-like ejecta. In addition, t…

astro-ph.SR202215 cited

Revisiting the evolved hypergiants in the Magellanic Clouds

Michalis Kourniotis, Michaela Kraus, Olga Maryeva +2

The massive stars that survive the phase of red supergiants (RSGs) spend the rest of their life in extremity. Their unstable atmospheres facilitate the formation and episodic eject…