Inward Bound: Studying the Galactic Centre with NAOS/CONICA
We report on the first results obtained using adaptive optics measurements of the Galactic Centre done with NAOS/CONICA.
10 results shown from 48 candidates · 616 indexed matches
We report on the first results obtained using adaptive optics measurements of the Galactic Centre done with NAOS/CONICA.
Structure of a quasi-stationary stellar cluster is modelled assuming that it is embedded in the gravitational field of a super-massive
The Infrared Space Observatory Long wavelength Spectrometerhas been used to map distribution of the emission from a sample of 22
The huge supergiant shell (SGS) LMC4, next to the giant HII region 30 Doradus the second most impressive feature of
OH(1720 MHz) masers permit direct measurements of the magnetic field strength at the Galactic Centre, and their angular broadening constrains
For many years it was felt that, when a star collapsed, a white dwarf resulted if the mass of the