Dusty star-forming galaxies at high redshift
Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …
Planck 2013 results. XI. All-sky model of thermal dust emission
A Abergel, PAR Ade, N Aghanim, MIR Alves… - Astronomy & …, 2014 - aanda.org
This paper presents an all-sky model of dust emission from the Planck 353, 545, and 857
GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky …
GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky …
Andromeda's dust
BT Draine, G Aniano, O Krause, B Groves… - The Astrophysical …, 2013 - iopscience.iop.org
ABSTRACT Spitzer Space Telescope and Herschel Space Observatory imaging of M31 is
used, with a physical dust model, to construct maps of dust surface density, dust-to-gas ratio …
used, with a physical dust model, to construct maps of dust surface density, dust-to-gas ratio …
The global dust SED: tracing the nature and evolution of dust with DustEM
M Compiègne, L Verstraete, A Jones… - Astronomy & …, 2011 - aanda.org
The Planck and Herschel missions are currently measuring the far-infrared to millimeter
emission of dust, which combined with existing IR data, will for the first time provide the full …
emission of dust, which combined with existing IR data, will for the first time provide the full …
Cluster-formation in the Rosette molecular cloud at the junctions of filaments
N Schneider, T Csengeri, M Hennemann… - Astronomy & …, 2012 - aanda.org
Aims. For many years feedback processes generated by OB-stars in molecular clouds,
including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to …
including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to …
The anatomy of the Orion B giant molecular cloud: A local template for studies of nearby galaxies
Context. Molecular lines and line ratios are commonly used to infer properties of extra-
galactic star forming regions. The new generation of millimeter receivers almost turns every …
galactic star forming regions. The new generation of millimeter receivers almost turns every …
A Herschel view of the far-infrared properties of submillimetre galaxies
B Magnelli, D Lutz, P Santini, A Saintonge… - Astronomy & …, 2012 - aanda.org
We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based
surveys, with known spectroscopic redshifts and observed with the Herschel Space …
surveys, with known spectroscopic redshifts and observed with the Herschel Space …
Herschel-Planck dust optical-depth and column-density maps-I. Method description and results for Orion
We present high-resolution, high dynamic range column-density and color-temperature
maps of the Orion complex using a combination of Planck dust-emission maps, Herschel …
maps of the Orion complex using a combination of Planck dust-emission maps, Herschel …
What does a submillimeter galaxy selection actually select? The dependence of submillimeter flux density on star formation rate and dust mass
CC Hayward, D Kereš, P Jonsson… - The Astrophysical …, 2011 - iopscience.iop.org
We perform three-dimensional dust radiative transfer (RT) calculations on hydrodynamic
simulations of isolated and merging disk galaxies in order to quantitatively study the …
simulations of isolated and merging disk galaxies in order to quantitatively study the …
What determines the density structure of molecular clouds? A case study of Orion B with Herschel
N Schneider, P André, V Könyves… - The Astrophysical …, 2013 - iopscience.iop.org
ABSTRACT A key parameter to the description of all star formation processes is the density
structure of the gas. In this Letter, we make use of probability distribution functions (PDFs) of …
structure of the gas. In this Letter, we make use of probability distribution functions (PDFs) of …