Search Publications

GOODS-Herschel: an infrared main sequence for star-forming galaxies
DOI: 10.1051/0004-6361/201117239 Bibcode: 2011A&A...533A.119E

Magnelli, B.; Lutz, D.; Altieri, B. +52 more

We present the deepest 100 to 500 µm far-infrared observations obtained with the Herschel Space Observatory as part of the GOODS-Herschel key program, and examine the infrared (IR) 3-500 µm spectral energy distributions (SEDs) of galaxies at 0 < z < 2.5, supplemented by a local reference sample from IRAS, ISO, Spitzer, and AKARI …

2011 Astronomy and Astrophysics
AKARI Herschel ISO eHST 1004
Modeling the evolution of infrared galaxies: a parametric backward evolution model
DOI: 10.1051/0004-6361/201015841 Bibcode: 2011A&A...529A...4B

Dole, H.; Lagache, G.; Béthermin, M. +2 more


Aims: We attempt to model the infrared galaxy evolution in as simple a way as possible and reproduce statistical properties such as the number counts between 15 µm and 1.1 mm, the luminosity functions, and the redshift distributions. We then use the fitted model to interpret observations from Spitzer, AKARI, BLAST, LABOCA, AzTEC, SPT, a…

2011 Astronomy and Astrophysics
AKARI Herschel 138
Mapping the radial structure of AGN tori
DOI: 10.1051/0004-6361/201117367 Bibcode: 2011A&A...536A..78K

Hönig, S. F.; Kishimoto, M.; Tristram, K. R. W. +3 more

We present mid-IR interferometric observations of six type 1 AGNs at multiple baseline lengths ranging from 27 m to 130 m, reaching high angular resolutions up to λ/B ~ 0.02 arcsec. For two of the targets, we have simultaneous near-IR interferometric measurements as well, taken within a week. We find that all the objects are partially resolved at …

2011 Astronomy and Astrophysics
AKARI 135
MESS (Mass-loss of Evolved StarS), a Herschel key program
DOI: 10.1051/0004-6361/201015829 Bibcode: 2011A&A...526A.162G

Ivison, R. J.; Blommaert, J. A. D. L.; Olofsson, G. +39 more

MESS (Mass-loss of Evolved StarS) is a guaranteed time key program that uses the PACS and SPIRE instruments on board the Herschel space observatory to observe a representative sample of evolved stars, that include asymptotic giant branch (AGB) and post-AGB stars, planetary nebulae and red supergiants, as well as luminous blue variables, Wolf-Rayet…

2011 Astronomy and Astrophysics
AKARI Herschel ISO 122
Planck early results. XXII. The submillimetre properties of a sample of Galactic cold clumps
DOI: 10.1051/0004-6361/201116481 Bibcode: 2011A&A...536A..22P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +201 more

We perform a detailed investigation of sources from the Cold Cores Catalogue of Planck Objects (C3PO). Our goal is to probe the reliability of the detections, validate the separation between warm and cold dust emission components, provide the first glimpse at the nature, internal morphology and physical characterictics of the Planck-detected sourc…

2011 Astronomy and Astrophysics
AKARI Herschel Planck 95
The outburst and nature of two young eruptive stars in the North America/Pelican Nebula Complex
DOI: 10.1051/0004-6361/201016160 Bibcode: 2011A&A...527A.133K

Pál, A.; Ábrahám, P.; Kóspál, Á. +8 more

Context. The sudden optical brightening of two young stellar objects, HBC 722 and VSX J205126.1+440523, located in the North America/Pelican Nebula Complex, was announced in August 2010. Early photometric and spectroscopic observations of these objects indicated that they may belong to the FUor or EXor class of young eruptive stars. The eruptions …

2011 Astronomy and Astrophysics
AKARI 83
Spectral energy distributions of an AKARI-SDSS-GALEX sample of galaxies
DOI: 10.1051/0004-6361/201015944 Bibcode: 2011A&A...529A..22B

Buat, V.; Burgarella, D.; Noll, S. +5 more

Context. The nearby universe remains the best laboratory to understand the physical properties of galaxies and is a reference for any comparison with high redshift observations. The all sky (or very large) surveys that have been performed from the ultraviolet (UV) to the far-infrared (far-IR) provide us with large datasets of very large wavelength…

2011 Astronomy and Astrophysics
AKARI 64
GOODS-Herschel: the impact of galaxy-galaxy interactions on the far-infrared properties of galaxies
DOI: 10.1051/0004-6361/201117476 Bibcode: 2011A&A...535A..60H

Magnelli, B.; Altieri, B.; Aussel, H. +15 more


Aims: We study the impact of galaxy-galaxy interactions on the far-infrared properties of galaxies and its evolution at 0 < z < 1.2.
Methods: Using the high-z galaxies in the fields of Great Observatories Origins Deep Survey (GOODS) observed by the Herschel Space Observatory in the framework of the GOODS-Herschel key program and th…

2011 Astronomy and Astrophysics
AKARI Herschel 52
A Herschel resolved far-infrared dust ring around HD 207129
DOI: 10.1051/0004-6361/201116673 Bibcode: 2011A&A...529A.117M

Fridlund, M.; Krivov, A. V.; Eiroa, C. +26 more

Context. Dusty debris discs around main sequence stars are thought to be the result of continuous collisional grinding of planetesimals in the system. The majority of these systems are unresolved and analysis of the dust properties is limited by the lack of information regarding the dust location.
Aims: The Herschel DUNES key program is obser…

2011 Astronomy and Astrophysics
AKARI Herschel 47
Herschel discovery of a new class of cold, faint debris discs
DOI: 10.1051/0004-6361/201117797 Bibcode: 2011A&A...536L...4E

Heras, A. M.; Fridlund, M.; Krivov, A. V. +25 more

We present Herschel PACS 100 and 160 µm observations of the solar-type stars α Men, HD 88230 and HD 210277, which form part of the FGK stars sample of the Herschel open time key programme (OTKP) DUNES (DUst around NEarby Stars). Our observations show small infrared excesses at 160 µm for all three stars. HD 210277 also shows a small ex…

2011 Astronomy and Astrophysics
AKARI Herschel 42