14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.2k papers
- California Institute of TechnologyUS1k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR744 papers
- University of CambridgeGB676 papers
- University College LondonGB641 papers
- University of TorontoCA603 papers
- National Institute for AstrophysicsIT595 papers
- Sapienza University of RomeIT578 papers
- Stanford UniversityUS550 papers
- European Southern ObservatoryCL540 papers
- Jet Propulsion LaboratoryUS533 papers
- University of ManchesterGB523 papers
13 papers · 2 filters
A Cool Dust Factory in the Crab Nebula: A Herschel Study of the Filaments
H. L. Gomez, O. Krause, M. J. Barlow +13
Whether supernovae are major sources of dust in galaxies is a long-standing debate. We present infrared and submillimeter photometry and spectroscopy from the Herschel Space Observ…
The JCMT Gould Belt Survey: SCUBA-2 observations of radiative feedback in NGC1333
J. Hatchell, T. Wilson, E. Drabek +5
We present observations of NGC1333 from SCUBA-2 on JCMT, observed as a JCMT Gould Belt Survey pilot project during the shared risk campaign when the first of four arrays was instal…
The Arecibo Galaxy Environment Survey VI : The Virgo Cluster (II)
R. Taylor, J. I. Davies, R. Auld +2
We present 21 cm observations of a 5 x degree region in the Virgo cluster, obtained as part of the Arecibo Galaxy Environment Survey. 13 cluster members are detected, together with…
Episodic accretion, protostellar radiative feedback, and their role in low-mass star formation
Dimitris Stamatellos, Anthony P. Whitworth, David A. Hubber
Protostars grow in mass by accreting material through their discs, and this accretion is initially their main source of luminosity. The resulting radiative feedback heats the envir…
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…
Dispersal of molecular clouds by ionising radiation
S. Walch, A. P. Whitworth, T. Bisbas +2
The role of feedback from massive stars is believed to be a key element in the evolution of molecular clouds. We use high-resolution 3D SPH simulations to explore the dynamical eff…
A Corona Australis cloud filament seen in NIR scattered light. III. Modelling and comparison with Herschel sub-millimetre data
M. Juvela, V. -M. Pelkonen, G. J. White +3
With recent Herschel observations, the northern filament of the Corona Australis cloud has now been mapped in a number of bands from 1.2um to 870um. The data set provides a good st…
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…
A search for pre-substellar cores and proto-brown dwarf candidates in Taurus: multiwavelength analysis in the B213-L1495 clouds
Aina Palau, I. de Gregorio-Monsalvo, Ò. Morata +9
In an attempt to study whether the formation of brown dwarfs (BDs) takes place as a scaled-down version of low-mass stars, we conducted IRAM30m/MAMBO-II observations at 1.2 mm in a…
The Resolved Stellar Population in 50 Regions of M83 from HST/WFC3 Early Release Science Observations
Hwihyun Kim, Bradley C. Whitmore, Rupali Chandar +22
We present a multi-wavelength photometric study of ~15,000 resolved stars in the nearby spiral galaxy M83 (NGC5236, D=4.61Mpc) based on Hubble Space Telescope Wide Field Camera 3 o…
Cluster-formation in the Rosette molecular cloud at the junctions of filaments
N. Schneider, T. Csengeri, M. Hennemann +31
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 trigger su…
The Pipe Nebula as seen with Herschel: Formation of filamentary structures by large-scale compression ?
N. Peretto, Ph. Andre, V. Konyves +20
A growing body of evidence indicates that the formation of filaments in interstellar clouds is a key component of the star formation process. In this paper, we present new Herschel…
The JCMT Legacy Survey of the Gould Belt: mapping 13CO and C18O in Orion A
J. V. Buckle, C. J. Davis, J. Di Francesco +31
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using HARP (Heterodyne Array Receiver Programme), SCUBA-2 (Submillimetre Common-User Bolometer Array 2) an…