activity
20052026
most citedThe IMF in Extreme Star-Forming Environments: Searching for Variations vs. Initial Conditions

3 citations · 6 across the 5 of their papers we have counts for

collaborators

5 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.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…

astro-ph.SR2025★ 3 cited

Substellar Initial Mass Function of Trumpler 14

Tamara Rom, Estelle Moraux, Koraljka Mužić +3

Young, massive stellar clusters offer a prime setting to explore brown dwarf (BD) formation under high densities and intense UV radiation. Trumpler 14 (Tr 14), a 1 Myr-old cluster…

astro-ph.GA2025

Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR). II. The initial mass function

M. Andersen, A. Brizawasi, Y. Cheng +5

To fully understand the star formation process, we are compelled to study it in a variety of environments. Of particular interest are how star formation and the resulting initial m…

astro-ph2005★ 3 cited

The IMF in Extreme Star-Forming Environments: Searching for Variations vs. Initial Conditions

Morten Andersen, M. R. Meyer, J. Greissl +4

Any predictive theory of star formation must explain observed variations (or lack thereof) in the initial mass function. Recent work suggests that we might expect quantitative vari…