36 citations · 57 across the 5 of their papers we have counts for
5 papers
A wide-field, multi-line survey of CO in the Magellanic Clouds at parsec-scale resolution: characterising the molecular gas content with a 50-m single-dish submillimeter telescope
Francisca Kemper, Rosie Chen, Axel Weiss +8
The Large and Small Magellanic Clouds (LMC, SMC) are nearby dwarf galaxies whose proximity uniquely enables molecular cloud-scale resolution observations across the entire Magellan…
A radial decrease in kinetic temperature measured with formaldehyde in 30 Doradus
Remy Indebetouw, Tony Wong, Suzanne Madden +4
Feedback from star formation is a critical component of the evolution of galaxies and their interstellar medium. At parsec scales internal to molecular clouds, however, the observe…
Observing the LMC with APEX: Signatures of Large-scale Feedback in the Molecular Clouds of 30 Doradus
Konstantin Grishunin, Axel Weiss, Dario Colombo +9
Stellar feedback plays a crucial role in star formation and the life cycle of molecular clouds. The intense star formation region 30 Doradus, which is located in the Large Magellan…
Molecular gas in the outflow of the Small Magellanic Cloud
Enrico M. Di Teodoro, N. M. McClure-Griffiths, C. De Breuck +7
We report the first evidence of molecular gas in two atomic hydrogen (HI) clouds associated with gas outflowing from the Small Magellanic Cloud (SMC). We used the Atacama Pathfinde…
Submillimeter Line Emission from LMC N159W: a Dense, Clumpy PDR in a Low Metallicity Environment
J. L. Pineda, N. Mizuno, J. Stutzki +30
Star formation at earlier cosmological times takes place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation…