179 citations · 1.6k across the 37 of their papers we have counts for
6 papers · 1 filter
Disentangling the circumnuclear environs of Centaurus A: II. On the nature of the broad absorption line
D. Espada, A. B. Peck, S. Matsushita +9
We report on atomic gas (HI) and molecular gas (as traced by CO(2-1)) redshifted absorption features toward the nuclear regions of the closest powerful radio galaxy, Centaurus A (N…
HIFI spectroscopy of low-level water transitions in M82
A. Weiss, M. A. Requena-Torres, R. Guesten +23
We present observations of the rotational ortho-water ground transition, the two lowest para-water transitions, and the ground transition of ionised ortho-water in the archetypal s…
Herschel observations of water vapour in Markarian 231
E. González-Alfonso, J. Fischer, K. Isaak +32
The Ultra Luminous InfraRed Galaxy Mrk 231 reveals up to seven rotational lines of water (H2O) in emission, including a very high-lying (E_{upper}=640 K) line detected at a 4sigma…
100 mum and 160 mum emission as resolved star-formation rate estimators in M33 (HERM33ES)
M. Boquien, D. Calzetti, C. Kramer +17
Over the past few years several studies have provided estimates of the SFR (star-formation rate) or the total infrared luminosity from just one infrared band. However these relatio…
The Herschel revolution: unveiling the morphology of the high mass star formation sites N44 and N63 in the LMC
S. Hony, F. Galliano, S. C. Madden +20
We study the structure of the medium surrounding sites of high-mass star formation to determine the interrelation between the HII regions and the environment from which they were f…
The Molecular Interstellar Medium of the Local Group Dwarf NGC6822
P. Gratier, J. Braine, N. J. Rodriguez-Fernandez +4
Do molecular clouds collapse to form stars at the same rate in all environments? In large spiral galaxies, the rate of transformation of H2 into stars (hereafter SFE) varies little…