312 citations · 724 across the 5 of their papers we have counts for
7 papers
High-mass star formation triggered by collision between CO filaments in N159 West in the Large Magellanic Cloud
Yasuo Fukui, Ryohei Harada, Kazuki Tokuda +20
We have carried out 13CO(J=2-1) observations of the active star-forming region N159 West in the LMC with ALMA. We have found that the CO distribution at a sub-pc scale is highly el…
The Herschel Dwarf Galaxy Survey: I. Properties of the low-metallicity ISM from PACS spectroscopy
D. Cormier, S. C. Madden, V. Lebouteiller +17
The far-infrared (FIR) lines are key tracers of the physical conditions of the interstellar medium (ISM) and are becoming workhorse diagnostics for galaxies throughout the universe…
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…
Dust continuum emission as a tracer of gas mass in galaxies
Brent A. Groves, Eva Schinnerer, Adam Leroy +8
We use a sample of 36 galaxies from the KINGFISH (Herschel IR), HERACLES (IRAM CO), and THINGS (VLA HI) surveys to study empirical relations between Herschel infrared (IR) luminosi…
Cool dust heating and temperature mixing in nearby star-forming galaxies
L. K. Hunt, B. T. Draine, S. Bianchi +20
Physical conditions of the interstellar medium in galaxies are closely linked to the ambient radiation field and the heating of dust grains. In order to characterize dust propertie…
Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation
Matthieu Béthermin, Emanuele Daddi, Georgios Magdis +17
We aim to measure the average dust and molecular gas content of massive star-forming galaxies () up to z=4 in the COSMOS field to determine if the…