Hot spots (HSs) are regions of enhanced radio emission produced by supersonic jets at the tip of the radio lobes of powerful radio sources. Obtained with the Very Large Telescope (VLT), images of the HSs in the radio galaxy 3C 445 show bright knots embedded in diffuse optical emission distributed along the post-shock region created by the impact of
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Particle Accelerators in the Hot Spots of Radio Galaxy 3C 445, Imaged with the VLTPrieto, M. A. et al.102002
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Particle-flow reconstruction and global event description with the CMS detector
The CMS apparatus was identified, a few years before the start of the LHC operation at CERN, to feature properties well suited to particle-flow (PF) reconstruction: a highly-segmented tracker, a fine-grained electromagnetic calorimeter, a hermetic hadron calorimeter, a strong magnetic field, and an excellent muon spectrometer. A fully-fledged PF
Sirunyan, A. M. et al.Advertised on:
102017 -
PASS: An All Sky Survey for the Detection of Transiting Extrasolar Planets and for Permanent Variable Star Tracking
An overview is given of the Permanent All Sky Survey (PASS) project. The primary goal of PASS is the detection of all transiting giant planets in the entire sky, complete for stellar systems of magnitudes ~5.5-10.5. Since the sample stars are fairly bright and relatively close, planets detected by PASS would be ideally suited for any follow-up
Deeg, H. J. et al.Advertised on:
102004 -
Past, present and future of cosmic microwave background observations: implications for cosmology
Not Available
Rubiño-Martin, J. A.Advertised on:
102008 -
Pattern Speeds of Bars and Spiral Arms from Hα Velocity Fields
We have applied the Tremaine-Weinberg method to 10 late-type barred spiral galaxies using data cubes, in Hα emission, from the FaNTOmM and GHAFAS Fabry-Perot spectrometers. We have combined the derived bar (and/or spiral) pattern speeds with angular frequency plots to measure the corotation radii for the bars in these galaxies. We base our results
Fathi, K. et al.Advertised on:
102009 -
PCA Inversions for the Rotation of the Solar Radiative Interior
Not Available
Eff-Darwich, A. et al.Advertised on:
102004