collaborators

8 papers

astro-ph.GA2026

EWOCS-VIII: Internal kinematics and expansion of Westerlund 1 from VVVX proper motions

C. Ordenes-Huanca, A. Bayo, M. Guarcello +12

Westerlund 1 (Wd1) is the most massive young star cluster known in the Milky Way and a key laboratory for studying the early dynamical evolution of massive clusters. Owing to its h…

astro-ph.IM2026

SHARPing accretion and outflows in young stellar objects in star forming regions of the outer Galaxy and beyond

Juan Manuel Alcala', Alessio Caratti o Garatti, Linda Podio +5

As part of the science book of SHARP, we present here the science case of star-disk interaction of low-mass (\Mstar2\Msun) young stellar objects (YSOs), in low-metallicity (Z…

astro-ph.IM2026

SHARP -- A spectrograph proposal to fully exploit ELT capabilities and look beyond JWST

P. Saracco, P. Conconi, C. Arcidiacono +47

The Extremely Large Telescopes (ELTs), with their large apertures and cutting-edge Multi-Conjugate Adaptive Optics (MCAO) systems, promise to deliver data that is both sharper and…

astro-ph.SR2026

EWOCS-VI: Probing the hidden intermediate-mass population of Westerlund 1

C. Ordenes-Huanca, A. Bayo, M. Guarcello +11

Context: Westerlund 1 (Wd1), the most massive young star cluster in the Milky Way, is an excellent laboratory for studying star formation and early stellar evolution in a starburst…

physics.plasm-ph2026

Experimental evidence for coronal mass ejection suppression in strong stellar magnetic fields

S. N. Chen, K. Burdonov, W. Yao +10

Solar coronal mass ejections (CME) are routinely observed, but as of yet there exist few convincing detections of stellar CMEs. A reason for this could be the stronger magnetic fie…

astro-ph.IM2025

SHARP: Beyond JWST -- Revealing the galaxy birth and growth with the resolution of the ELT

P. Saracco, P. Conconi, C. Arcidiacono +37

A deep understanding of the life-cycle of galaxies, particularly those of high mass, requires clarifying the mechanisms that regulate star formation (SF) and its abrupt shutdown (q…