activity
20112015
most citedVarying [CII]/[NII] line ratios in the interacting system BR1202-0725 at z=4.7

59 citations · 112 across the 4 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2015★ 12 cited

Heating and cooling of the neutral ISM in the NGC4736 circumnuclear ring

T. P. R. van der Laan, L. Armus, P. Beirao +12

The manner in which gas accretes and orbits within circumnuclear rings has direct implications for the star formation process. In particular, gas may be compressed and shocked at t…

astro-ph.GA2014★ 6 cited

Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations

Juan R. Martínez-Galarza, Howard A. Smith, Lauranne Lanz +7

(abridged) The majority of star-forming galaxies follow a simple empirical correlation in the star formation rate (SFR) versus stellar mass () plane, usually referred to as th…

astro-ph.GA2014★ 35 cited

The metallicity of void dwarf galaxies

K. Kreckel, K. Croxall, B. Groves +2

The current Lambda CDM cosmological model predicts that galaxy evolution proceeds more slowly in lower density environments, suggesting that voids are a prime location to search fo…

astro-ph.GA2014★ 59 cited

Varying [CII]/[NII] line ratios in the interacting system BR1202-0725 at z=4.7

R. Decarli, F. Walter, C. Carilli +8

We study the properties of the interstellar medium in the interacting system BR1202-0725 at z=4.7 via its [NII] and [CII] fine-structure line emission. This system consists of a QS…

astro-ph.CO2012

Ongoing Massive Star Formation in NGC 604

Juan R. Martínez-Galarza, Deidre Hunter, Brent Groves +1

NGC 604 is the second most massive H II region in the Local Group, thus an important laboratory for massive star formation. Using a combination of observational and analytical tool…

astro-ph.CO2012

Cool Dust in the Outer Ring of NGC 1291

J. L. Hinz, C. W. Engelbracht, R. Skibba +18

We examine Herschel Space Observatory images of one nearby prototypical outer ring galaxy, NGC 1291, and show that the ring becomes more prominent at wavelengths longer than 160um.…