activity
20172026
most citedBinarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC

37 citations · 310 across the 35 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA20253 cited

SDSS-V LVM: Resolving Physical Conditions in the Trifid Nebula

Natascha Sattler, J. Eduardo Méndez-Delgado, Kathryn Kreckel +18

The chemical abundance of the interstellar medium sets the initial conditions for star formation and provides a probe of chemical galaxy evolution models. However, unresolved inhom…

astro-ph.GA20251 cited

Can Wolf-Rayet stars be the missing ingredient to explain high-z He II ionizing radiation?

G. González-Torà, A. A. C. Sander, E. Egorova +7

Classical Wolf-Rayet (WR) stars are hot, massive stars with depleted hydrogen. At low metallicities (Z), WN3-type WR stars have relatively thin winds and are major sources of ioniz…

astro-ph.GA2024

Chemical abundances and ionizing mechanisms in the star-forming double-ring of AM 0644-741 using MUSE data

V. M. A. Gómez-González, Y. D. Mayya, J. Zaragoza-Cardiel +6

We present the analysis of archival Very Large Telescope (VLT) Multi-Unit Spectroscopic Explorer (MUSE) observations of 179 HII regions in the star-forming double-ring collisional…

astro-ph.GA20235 cited

Looking for nebular He II emission south of the multiple-massive star system, HD 5980

Andres Sixtos, Aida Wofford, Andreas A. C. Sanders +1

The nebular He II λ1640 emission line is observed in star forming galaxies out to large distances and can be used to constrain the properties of sources of He+ ionizing photons. Fo…

astro-ph.GA20213 cited

A meeting at z~3: Young massive galaxies and an AGN within 30kpc of the luminous QSO LBQS0302-0019

B. Husemann, G. Worseck, F. Arrigoni Battaia +2

Contrary to expectations from scenarios of black hole growth driven by galaxy interactions and mergers, dual active galactic nuclei (AGN) with kiloparsec separations are rarely obs…

astro-ph.GA2018

Stellar population of the superbubble N206 in the LMC II. Parameters of the OB and WR stars, and the total massive star feedback

Varsha Ramachandran, W. -R. Hamann, R. Hainich +5

Clusters or associations of early-type stars are often associated with a 'superbubble' of hot gas. The formation of such superbubbles is caused by the feedback from massive stars.…