Centre of mass in spaces with torsion free flat linear connection
The concept "centre of mass" is analyzed in spaces with torsion free flat linear connection. It is shown that under
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The concept "centre of mass" is analyzed in spaces with torsion free flat linear connection. It is shown that under
Using the IRAM interferometer, we have observed the nearby starburst galaxy M82 with a 4.2" resolution (~70 pc) in the
We report observations at mid-infrared and sub-millimeter wavelengths of Centaurus A (CenA, NGC 5128), the giant elliptical galaxy that harbors
Sgr A* is currently being fed by winds from a cluster of gravitationally bound young mass-loosing stars. Using observational constraints
A comparison of the XMM-Newton and Chandra Galactic Centre (GC) Surveys has revealed two faint X-ray transients with contrasting properties.
The few central parsecs of the Galaxy are known to contain a surprising population of early-type stars, including at least
The now substantial evidence for a rotating bar in the inner Galaxy and its dynamical implications are reviewed.
We have measured deconfined hadronic volumes, 4.4 < V < 13.0 fm^3, produced by one-dimensional(1D) expansion. The volumes are directly
The radio source Sagittarius A* (Sgr A*), is thought to be a supermassive black hole located at the centre of
We present early results from the first IR imaging of the weak X-ray sources discovered in a recent Chandra survey
The multi-centre metrics are a family of euclidean solutions of the empty space Einstein equations with self-dual curvature. For this
We report on the first results obtained using adaptive optics measurements of the Galactic Centre done with NAOS/CONICA.
We carried out a systematic search for new star clusters in a field of 5$^{\circ} \times5^{\circ}$ centred close to the
The Infrared Space Observatory Long wavelength Spectrometerhas been used to map distribution of the emission from a sample of 22
OH(1720 MHz) masers permit direct measurements of the magnetic field strength at the Galactic Centre, and their angular broadening constrains
There are many observational evidences for the existence of massive compact condensations in the range $10^6 -10^{10} M_\odot$ at the
For many years it was felt that, when a star collapsed, a white dwarf resulted if the mass of the
ScotGrid is a prototype regional computing centre formed as a collaboration between the universities of Durham, Edinburgh and Glasgow as
We present initial results of a spectroscopic study of the Pistol and of the cocoon stars in the Quintuplet Cluster.
Structure of a quasi-stationary stellar cluster is modelled assuming that it is embedded in the gravitational field of a super-massive
We report the status of a search for pulsars in the Galactic Centre, using a completely revised and improved high-sensitivity
We have observed the central 45' region of the Galaxy at 620 MHz band of the Giant Metrewave Radio Telescope
The INTEGRAL Science Data Centre (ISDC) processes, archives and distributes data from the INTEGRAL mission. At the ISDC incoming data
The huge supergiant shell (SGS) LMC4, next to the giant HII region 30 Doradus the second most impressive feature of