Evolution of Globular Clusters Formed in Mergers
Globular clusters formed in galactic mergers (e.g., The Antennae) can now be studied at different stages of their evolution. In
43 indexed results
Globular clusters formed in galactic mergers (e.g., The Antennae) can now be studied at different stages of their evolution. In
A revised metallicity calibration of the Stroemgren (b-y),m_1 diagram, based on a sample of globular cluster and field red giant
Most Tidal Dwarf Galaxies (TDGs) so-far discussed in the literature may be considered as young ones or even newborns, as
Recent results on the detection of substructure in dwarf spheroidal galaxies are discussed. In most cases they show that, when
I review our observational and theoretical knowledge of AM CVn stars, focusing on recent developments. These include newly discovered systems,
With the 1998 announcement of new evidence for muon neutrino disappearance observed by the Super-Kamiokande experiment, the more than a
Gamma-ray bursts are sudden releases of energy that for a duration of a few seconds outshine even huge galaxies. 30
We present deep (I,V-I) and (I,B-I) color-magnitude diagrams (CMDs) of the Antlia dwarf galaxy, based on Science Verification (SV) data
In this article we briefly review our recent results on evolution and properties of isolated neutron stars (INSs) in the
Observations increasingly demonstrate the spatial association of high redshift objects with larger, low redshift galaxies. These companion objects show a
We present limits to the log N - log S curve for isolated neutron stars, both cooling and accreting neutron
High quality spectrophotometric observations of 30 Planetary Nebulae in the Galactic Bulge have been made. Accurate reddenings, plasma parameters, and
The last decade of research on elliptical galaxies has produced a wealth of new information concerning both their detailed structure
Deep, wide-range and accurate UBVRI photometric sequences have been established around more than 80 symbiotic stars, to assist current photometry
Sgr A* is extra-ordinarily dim in all wavelengths requiring a very low accretion rate at the present time. However, at
In the common model supernova shock-acceleration of cosmic rays there are two open questions: 1. where does the high energy
Observations in integrated light (2200-4800 A, 8 to 11 A resolution, S/N > 20) of 4 M31 globular clusters and
I present the preliminary results of a program to measure the star formation history in the halo of the Andromeda
We present recent near-infrared detections of circumstellar disks around the two old PMS Herbig stars HD 141569 and HD 100546
We show that {\em ground-based} direct imaging detection of extra-solar planets is possible with current technology. As an example, we
To first order, the initial cluster luminosity function appears to be universal. This means that the brightest young cluster in
In this poster I discuss the nature of the compact X-ray source in the center of the supernova remnant RCW
We study the conceptual feasibility of a high energy, ``short baseline'', zero background experiment to search for muon-neutrino --> electron-neutrino
A fair and complete accounting of cosmic baryons now appears possible, because most of them are in states which are