activity
20072026
most citedAn Overview of the Dwarf Galaxy Survey

258 citations · 825 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2026

A multi-scale molecular and atomic gas view on the HII region N113 in the Large Magellanic Cloud:Evidence for high-mass star formation triggered by supersonically-colliding HI flows

Rin I. Yamada, Kazuki Tokuda, Yasuo Fukui +15

The Large Magellanic Cloud (LMC) exhibits vigorous high-mass star formation, including the HII regions 30~Dor that is the most active site of star formation in the local group. The…

astro-ph.GA2022★ 8 cited

Sequential Star Formation in the Young SMC Region NGC 602: Insights from ALMA

Theo J. O'Neill, Remy Indebetouw, Karin Sandstrom +7

NGC 602 is a young, low-metallicity star cluster in the "Wing" of the Small Magellanic Cloud. We reveal the recent evolutionary past of the cluster through analysis of high-resolut…

astro-ph.SR2019★ 17 cited

Herschel spectroscopy of Massive Young Stellar Objects in the Magellanic Clouds

J. M. Oliveira, J. Th. van Loon, M. Sewilo +11

We present Herschel Space Observatory Photodetector Array Camera and Spectrometer (PACS) and Spectral and Photometric Imaging Receiver Fourier Transform Spectrometer (SPIRE FTS) sp…

astro-ph.GA2019★ 25 cited

Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. II. 30 Doradus

Min-Young Lee, Suzanne Madden, Franck Le Petit +6

With an aim of probing the physical conditions and excitation mechanisms of warm molecular gas in individual star-forming regions, we performed Herschel SPIRE FTS observations of 3…

astro-ph.GA2016★ 22 cited

Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. I. N159W

Min-Young Lee, Suzanne Madden, Vianney Lebouteiller +25

We present Herschel SPIRE Fourier Transform Spectrometer (FTS) observations of N159W, an active star-forming region in the Large Magellanic Cloud (LMC). In our observations, a numb…

astro-ph.GA2015★ 48 cited

Star-formation rates from young-star counts and the structure of the ISM across the NGC346/N66 complex in the SMC

S. Hony, D. A. Gouliermis, F. Galliano +21

The rate at which interstellar gas is converted into stars, and its dependence on environment, is one of the pillars on which our understanding of the visible Universe is build. We…