Here is a state-of-the-art review of our current knowledge of brown dwarfs and very low-mass stars. The hunt for, and study of, these elusive objects is...
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...