activity
20052025
most citedLow-Frequency Radio Absorption in Cassiopeia A

46 citations · 473 across the 27 of their papers we have counts for

collaborators

27 papers

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

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…

astro-ph.SR2023★ 2 cited

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★ 7 cited

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.HE2022

Possible discovery of Calvera's supernova remnant

M. Arias, A. Botteon, C. G. Bassa +13

We report the discovery of a ring of low surface brightness radio emission around the Calvera pulsar, a high Galactic latitude, isolated neutron star, in the LOFAR Two-metre Sky Su…

astro-ph.SR2022★ 3 cited

Simultaneous J-, H-, K- and L-band spectroscopic observations of galactic Be stars. I. IR atlas

Y. R. Cochetti, M. L. Arias, L. S. Cidale +2

It is already accepted that Be stars are surrounded by circumstellar envelopes, which are mostly compatible with a disc geometry in Keplerian rotation. We aim to obtain a more comp…