activity
19992003
most citedA search for Symbiotic Stars in the Local Group

3 citations · 4 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph2003

Automated Determination of Stellar Population Parameters in Galaxies Using Active Instance-based Learning

Thamar Solorio, Olac Fuentes, Roberto Terlevich +2

In this work we focus on the determination of the relative distributions of young, intermediate-age and old populations of stars in galaxies. Starting from a grid of theoretical po…

astro-ph2003

Spectroscopy, Photometry and Micro-arcsec Astrometry of Binaries with the GAIA Space Mission and with the RAVE Experiment

Tomaz Zwitter, Ulisse Munari

GAIA astrometric mission of ESA will be very efficient in discovering binary and multiple stars with any orbital period, from minutes to millions of years. Main parameters of the r…

astro-ph20021 cited

Mass of BL Lacs from the Velocity Dispersion of the Host Galaxy

A. Treves, N. Carangelo, R. Falomo +1

We report on new measurements of the stellar velocity dispersion of 4 BL Lac objects for which optical spectroscopy was gathered at the ESO 3.6m using EFOSC2. Assuming the M(BH)--(…

astro-ph20023 cited

A search for Symbiotic Stars in the Local Group

Laura Magrini, Romano L. M. Corradi, Ulisse Munari

The Local Group Census is a narrow- and broad-band survey of all the galaxies of the Local Group above dec = -30 deg, in progress at the 2.5m Isaac Newton telescope on La Palma. We…

astro-ph2000

Spiral and irregular galaxies in the Hubble Deep Field North - Comparison with early types and implications for the global SFR density

G. Rodighiero, G. L. Granato, A. Franceschini +2

We analyze a morphologically-selected complete sample of 52 late-type (spiral and irregular) galaxies in the Hubble Deep Field North with total K-magnitudes brighter than K=20.47.…

astro-ph2000

The bright 175um knots of the Andromeda Galaxy

L. Schmidtobreick, M. Haas, D. Lemke

Discrete far-infrared (FIR) sources of M31 are identified in the ISO 175um map and characterized via their FIR colours, luminosities and masses. With a mean size of 800pc, they pro…