7.7k citations
- National Institute for AstrophysicsIT429 papers
- Centre National de la Recherche ScientifiqueFR378 papers
- Max Planck Institute for Radio AstronomyDE364 papers
- University of ManchesterGB254 papers
- Istituto di Radioastronomia di BolognaIT240 papers
- Commonwealth Scientific and Industrial Research OrganisationAU236 papers
- Netherlands Institute for Radio AstronomyNL231 papers
- Brera Astronomical ObservatoryIT219 papers
- Astronomical Observatory of RomeIT210 papers
- Center for Astrophysics Harvard & SmithsonianUS210 papers
- University of PaduaIT183 papers
- University of AmsterdamNL178 papers
17 papers · 1 filter
Molecular Superbubbles and Outflows from Starburst Galaxy NGC 2146
An-Li Tsai, Satoki Matsushita, Kouichiro Nakanishi +7
We present results from a deep (1 sigma = 5.7 mJy beam^{-1} per 20.8 km s^{-1} velocity channel) ^{12}CO(1-0) interferometric observation of the central 60" region of the nearby ed…
PSR J1753-2240: A mildly recycled pulsar in an eccentric binary system
M. J. Keith, M. Kramer, A. G. Lyne +5
We report the discovery of PSR J1753-2240 in the Parkes Multibeam Pulsar Survey database. This 95-ms pulsar is in an eccentric binary system with a 13.6-day orbital period. Period…
Double relics in Abell 2345 and Abell 1240: spectral index and polarization analysis
A. Bonafede, G. Giovannini, L. Feretti +2
The aim of the present work is to study the radio properties of double relics in Abell 1240 and Abell 2345 in the framework of double relic formation models. We present new Very La…
High-Resolution Timing Observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope
A. Pellizzoni, M. Pilia, A. Possenti +67
AGILE is a small gamma-ray astronomy satellite mission of the Italian Space Agency dedicated to high-energy astrophysics launched in 2007 April. Its 1 microsecond absolute time tag…
Structures of the magnetoionic media around the FR I radio galaxies 3C 31 and Hydra A
R. A. Laing, A. H. Bridle, P. Parma +1
We use high-quality VLA images of the Fanaroff & Riley Class I radio galaxy 3C 31 at six frequencies in the range 1365 to 8440MHz to explore the spatial scale and origin of the rot…
Dehydrogenated polycyclic aromatic hydrocarbons and UV bump
G. Malloci, G. Mulas, C. Cecchi-Pestellini +1
Recent calculations have shown that the UV bump at about 217.5 nm in the extinction curve can be explained by a complex mixture of PAHs in several charge states. Other studies prop…