187 citations · 1.2k across the 21 of their papers we have counts for
21 papers
Micro-turbulence across the Hertzsprung-Russell diagram. Observational constrains for stars in the MW
N. Markova, M. Cantiello, L. Grassitelli
We assemble a homogeneous database of precise and consistent determinations of effective temperature, surface gravity, projected rotational rate, and macro- and micro-turbulent vel…
Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
Yvonne A. Fichtner, Jonathan Mackey, Luca Grassitelli +2
Energy and momentum feedback from stars is a key element of models for galaxy formation and interstellar medium dynamics, but resolving the relevant length scales to directly inclu…
X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description
Jorick S. Vink, A. Mehner, P. A. Crowther +78
Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts, and gravitational-wave events involving spectacular black-hole mergers, indicate that the low…
Bringing Stellar Evolution & Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022
Sam Geen, Poojan Agrawal, Paul A. Crowther +34
Stars strongly impact their environment, and shape structures on all scales throughout the universe, in a process known as ``feedback''. Due to the complexity of both stellar evolu…
Inverse Compton cooling of thermal plasma in colliding-wind binaries
Jonathan Mackey, Thomas A. K. Jones, Robert Brose +3
The inverse-Compton effect (IC) is a widely recognized cooling mechanism for both relativistic and thermal electrons in various astrophysical environments, including the intergalac…
Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
Yvonne A. Fichtner, Luca Grassitelli, Emilio Romano-Díaz +1
We compute different sets of stellar evolutionary tracks in order to quantify the energy, mass, and metals yielded by massive main-sequence and post-main-sequence winds. Our aim is…