Recent studies have claimed the existence of very massive stars (VMS) up to 300 M ⊙ in the local Universe. As this finding may represent a paradigm shift for...
Very Small Array. Flux density at 33GHz (Cleary+, 2005)
We describe the source subtraction strategy and observations for the extended Very Small Array (VSA), a cosmic microwave background interferometer operating at...
Very Small Array. Flux density at 33GHz (Cleary+, 2005)
We describe the source subtraction strategy and observations for the extended Very Small Array (VSA), a cosmic microwave background interferometer operating at...
Very Small Array. II. CMB at 34GHz (Taylor+, 2003)
We have observed the cosmic microwave background (CMB) temperature fluctuations in eight fields covering three separated areas of sky with the Very Small Array...
Very-High-Energy γ-Ray Observations of a Strong Flaring Activity in M 87 in 2008 February
M 87 is the only known non blazar radio galaxy to emit very high energy (VHE) gamma-rays. During a monitoring program of M 87, a rapid flare in VHE gamma-rays...
Very-high-energy γ-rays from the universe middle age: Detection of B0218+357 and PKS1441+25 with the MAGIC telescopes
Out of the ˜ 70 extragalactic sources known to emit in the Very High Energy band (VHE, E > 100GeV), only 5-6 are known to be Flat Spectrum Radio Quasars (FSRQs)...
Vestige of a Beginning: a Quest for 142Nd Anomalies in the Earth
Although seismic tomography evidence leaves no room for fully layered mantle convection, it is still arguable that over Earth's history convection has...
Vestoids and V-type asteroids: A Mineralogical Characterization.
Asteroid (4) Vesta is known as the unique large object of the main belt showing a basaltic crust and is a target of the NASA Dawn Mission. Vesta composition is...