Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR14k papers
- Centre National de la Recherche ScientifiqueFR9.8k papers
- Université Paris-SaclayFR5.1k papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR5k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR3.8k papers
- Astrophysique, Instrumentation et ModélisationFR3.3k papers
- Université Paris CitéFR3.3k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT2.4k papers
- European Organization for Nuclear ResearchCH2.4k papers
- The Ohio State UniversityUS2.3k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT2.3k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT2.2k papers
20 papers · 2 filters
A First Look at the Auriga-California Giant Molecular Cloud With Herschel and the CSO: Census of the Young Stellar Objects and the Dense Gas
Paul M. Harvey, Cassandra Fallscheer, Adam Ginsburg +7
We have mapped the Auriga/California molecular cloud with the Herschel PACS and SPIRE cameras and the Bolocam 1.1 mm camera on the Caltech Submillimeter Observatory (CSO) with the…
Changes Of Dust Opacity With Density in the Orion A Molecular Cloud
Arabindo Roy, Peter G. Martin, Danae Polychroni +12
We have studied the opacity of dust grains at submillimeter wavelengths by estimating the optical depth from imaging at 160, 250, 350, and 500 um from the Herschel Gould Belt Surve…
Recent star formation in the Lupus clouds as seen by Herschel
K. L. J. Rygl, M. Benedettini, E. Schisano +26
We present a study of the star formation histories of the Lupus I, III, and IV clouds using the Herschel 70-500 micron maps obtained by the Herschel Gould Belt Survey Key Project.…
Traces of past activity in the Galactic Centre
Gabriele Ponti, Mark R. Morris, Regis Terrier +1
The Milky Way centre hosts a supermassive Black Hole (BH) with a mass of ~4*10^6 M_Sun. Sgr A*, its electromagnetic counterpart, currently appears as an extremely weak source with…
Herschel observations of B1-bS and B1-bN: two first hydrostatic core candidates in the Perseus star-forming cloud
Stefano Pezzuto, D. Elia, E. Schisano +24
We report far-IR Herschel observations obtained between 70 m and 500 m of two star-forming dusty condensations, B1-bS and B1-bN, in the B1 region of the Perseus star-forming…
Interstellar matter and star formation in W5-E - A Herschel view
L. Deharveng, A. Zavagno, L. D. Anderson +7
W5-E has been observed with the Herschel-PACS and -SPIRE photometers, at 100, 160, 250, 350, and 500 microns. The dust temperature map shows a rather uniform temperature, in the ra…
The nature of the interstellar medium of the starburst low-metallicity galaxy Haro11: a multi-phase model of the infrared emission
D. Cormier, V. Lebouteiller, S. C. Madden +15
(abridged) Our goal is to describe the multi-phase ISM of the IR bright low-metallicity galaxy Haro 11, dissecting the photoionised and photodissociated gas components. We present…
Submillimetre line spectrum of the Seyfert galaxy NGC1068 from the Herschel-SPIRE Fourier Transform Spectrometer
Luigi Spinoglio, Miguel Pereira-Santaella, Gemma Busquet +13
The first complete submillimetre spectrum (190-670um) of the Seyfert 2 galaxy NGC1068 has been observed with the SPIRE Fourier Transform Spectrometer onboard the {\it Herschel} Spa…
Planck Intermediate Results. IX. Detection of the Galactic haze with Planck
Planck Collaboration, P. A. R. Ade, N. Aghanim +181
Using precise full-sky observations from Planck, and applying several methods of component separation, we identify and characterize the emission from the Galactic "haze" at microwa…
The Earliest Phases of Star Formation (EPoS): A Herschel Key Program - The precursors to high-mass stars and clusters
Sarah Ragan, Thomas Henning, Oliver Krause +14
(Abridged) We present an overview of the sample of high-mass star and cluster forming regions observed as part of the Earliest Phases of Star Formation (EPoS) Herschel Guaranteed T…
The H2O southern Galactic Plane Survey(HOPS): NH3 (1,1) and (2,2) catalogues
C. R. Purcell, S. N. Longmore, A. J. Walsh +19
The H2O Southern Galactic Plane Survey (HOPS) has mapped a 100 degree strip of the Galactic plane (-70deg > l > 30deg, |b| < 0.5deg) using the 22-m Mopra antenna at 12-mm wavelengt…
Interferometric Identification of a Pre-Brown Dwarf
Philippe André, Derek Ward-Thompson, Jane Greaves
It is not known whether brown dwarfs (stellar-like objects with masses less than the hydrogen-burning limit, 0.075 Msun) are formed in the same way as solar-type stars or by some o…
The two-phase formation history of spiral galaxies traced by the cosmic evolution of the bar fraction
Katarina Kraljic, Frédéric Bournaud, Marie Martig
We study the evolution of galactic bars and the link with disk and spheroid formation in a sample of zoom-in cosmological simulations. Our simulation sample focuses on galaxies wit…
Profiling filaments: comparing near-infrared extinction and submillimetre data in TMC-1
J. Malinen, M. Juvela, M. G. Rawlings +3
Interstellar filaments are an important part of star formation. To understand the structure of filaments, cross-section profiles are often fitted with Plummer profiles. This profil…
The spine of the swan: A Herschel study of the DR21 ridge and filaments in Cygnus X
M. Hennemann, F. Motte, N. Schneider +31
In order to characterise the cloud structures responsible for the formation of high-mass stars, we present Herschel observations of the DR21 environment. Maps of the column density…
Deep Silicate absorption features in Compton-thick AGN predominantly arise due to dust in the host galaxy
A. D. Goulding, D. M. Alexander, F. E. Bauer +5
We explore the origin of mid-infrared (mid-IR) dust extinction in all 20 nearby (z < 0.05) bona-fide Compton-thick (N_H > 1.5 x 10^24 cm^-2) AGN with hard energy (E > 10 keV) X-ray…
The Dust Properties of Bubble HII Regions as seen by Herschel
L. D. Anderson, A. Zavagno, L. Deharveng +10
Because of their relatively simple morphology, "bubble" HII regions have been instrumental to our understanding of star formation triggered by HII regions. With the far-infrared (F…
SOFIA observations of S106: Dynamics of the warm gas
Robert Simon, Nicola Schneider, Juergen Stutzki +6
Context. The HII region/PDR/molecular cloud complex S106 is excited by a single O-star. The full extent of the warm and dense gas close to the star has not been mapped in spectrall…
Galactic cold cores III. General cloud properties
M. Juvela, I. Ristorcelli, L. Pagani +15
We examine the cloud structure around the Planck detections in 71 fields observed with the Herschel SPIRE instrument. We wish to determine the general physical characteristics of t…
RAMSES-CH: A New Chemodynamical Code for Cosmological Simulations
C. Gareth Few, Stephanie Courty, Brad K. Gibson +3
We present a new chemodynamical code - Ramses-CH - for use in simulating the self-consistent evolution of chemical and hydrodynamical properties of galaxies within a fully cosmolog…