1.8 MeV Emission from the Carina Region
Significant 1.8 MeV emission from the Carina region has been detected by COMPTEL. The emission is concentrated within 6 degrees
16 indexed results
Significant 1.8 MeV emission from the Carina region has been detected by COMPTEL. The emission is concentrated within 6 degrees
We study the first microlensing event toward the Carina spiral arm discovered by the OGLE collaboration. We demonstrate that this
We report on the chemical abundances of stars in the Carina dwarf spheroidal galaxy (dSph) derived from low-resolution spectra. We
We present metallicities for 487 red giants in the Carina dwarf spheroidal (dSph) galaxy that were obtained from FLAMES low-resolution
We present photometry for stars in the Carina dwarf spheroidal galaxy that is unprecedented in depth, accuracy and spatial coverage.
Recent cosmological N-body simulations suggest that current empirical estimates of tidal radii in dSphs might be underestimated by at least
The re-analysis of the data reported by Mateo et al. (1998) allowed us to obtain a partially different set of
We present preliminary results from a detailed study towards four previously detected bright mid-infrared sources in the southern part of
We present results of a new investigation (Carraro et al. 2002) aimed at clarifying the mutual relationship between the most
We analyze the mean luminosity of three samples of field RRab Lyr stars observed in the course of the OGLE
Many past attempts to kill MOND have only strengthened the theory. Better data on galaxy velocity curves clearly favor MOND
The SPIREX telescope, located at the Amundsen-Scott South Pole Station, was a prototype system developed to exploit the excellent conditions
We have recalculated the orbits of 3 binary systems, members of the open cluster Trumpler 16 in the Carina region.
(Abridged) We present results of deep near-infrared JK imaging of LMC, SMC, and the Carina and Fornax dwarf galaxies. A
Pulsars provide unique probes for the {\it large-scale} interstellar magnetic field in the Galactic disk. The Parkes multibeam pulsar survey
BVI photometry of the Magellanic Clouds collected during the OGLE-II microlensing experiment makes it possible to study in detail photometric