Low-Degree High-Frequency p and g Modes in the Solar Core
Solar gravity (g) modes propagate within the radiative part of the solar interior and are highly sensitive to the physical conditions of the solar core. They...
We present new results of a program aimed at studying the physical properties, origin and evolution of those phenomena which go under the somewhat generic...
Low-level control software for the WEAVE spectrograph
WEAVE is a wide-field spectroscopy facility for WHT which includes a multi-object dual-beam spectrograph which will operate in the visible wavelength range. The...
Asymmetric Planetary Nebulae (APN) are formed by bipolar outflows through various mechanism like fast rotation (Blackman et al. 2001), magnetic field (Regos &...
Low-mass stars and brown dwarfs in Praesepe (Baker+, 2010)
Presented are the results of a large and deep optical-near-infrared multi-epoch survey of the Praesepe open star cluster using data from the UKIRT Infrared Deep...
The double distance and metallicity frontier marked by the SMC has been finally broken with the aid of powerful multi-object spectrographs installed at 8-10m...
LOWL p-mode frequencies and their variation with solar activity
We present an analysis of the frequency shift and the even terms of the frequency splitting coefficients carried out using six years of LOWL data, starting in...