collaborators

6 papers

astro-ph.SR2026

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants

Lydia S. Cidale, Alejandra Christen, Aldana Alberici Adam +6

The properties of O-type supergiant stars remain largely unexplored. By analysing their light variations, we can unravel underlying physical phenomena, such as binarity, stellar pu…

astro-ph.SR2026

An Halpha survey of infrared bow-shocks around OB-type stars

Kuljeet Singh Saddal, Michaela Kraus, Dieter H. Nickeler +3

Bow shocks (BSs) around massive stars are commonly identified in mid-infrared (MIR) surveys. In contrast, systematic optical investigations of these structures remain scarce with o…

astro-ph.SR2026

High-resolution near-IR spectroscopy of the B[e] supergiant LHA 115-S 18: discovery of hot water vapor emission

M. L. Arias, A. F. Torres, M. Kraus +1

The post-main-sequence evolution of massive stars involves phases of intense, often eruptive mass loss, including the B[e] supergiant phase. These hot stars are surrounded by cool,…

astro-ph.SR2025

Near-infrared characterization of evolved massive stars in M31 and M33

Michaela Kraus, Maria Laura Arias, Michalis Kourniotis +3

The upper region of the Hertzsprung-Russell diagram is populated by massive stars in a diversity of evolutionary stages, and the classification of these stars is often based on obs…

astro-ph.SR2025

Variability of Galactic blue supergiants observed with TESS

Michalis Kourniotis, Lydia S. Cidale, Michaela Kraus +2

Blue supergiants (BSGs) mediate between the main sequence and the late stages of massive stars, which makes them valuable for assessing the physics that drives the stars across the…

astro-ph.SR2025

HD 144812: A transition-phase massive star in a binary system

Michalis Kourniotis, Michaela Kraus, Maria Laura Arias +1

In this Letter, we shed light on the evolutionary phase of HD 144812, a Galactic yellow supergiant showing infrared excess that is typically expected for evolved stars undergoing e…