Multi-object spectroscopic observations of A697 were carried out at the TNG telescope in December 2003 during the program of proposal AOT8/CAT-G6. (1 data file).

By detecting ionised-gas emission in 75% of the cases, the SAURON integral-field spectroscopic survey has further demonstrated that early-type galaxies often display nebular emission. Furthermore, the SAURON data have shown that such emission comes with an intriguing variety of morphologies, kinematic behaviours and line ratios. Perhaps most

We present deep, high angular-resolution HST NICMOS imaging in the Hubble Deep Field South (HDF-S), focusing on a subset of 14 distant red galaxies (DRGs) at z~2.5 that have been preselected to have J-K>2.3. We find a clear trend between the rest-frame optical sizes of these sources and their luminosity-weighted stellar ages as inferred from their

We report the discovery of a new X-ray source detected in a 5ks observation starting on 2007-02-14.08 UT as part of our ongoing Chandra/HST M31 transient program. The source was detected at coordinates RA(J2000) 00:44:12.4, Dec(J2000) 41:25:48.2, at the edge of the ACIS-S field of view, which results in larger than usual position errors of 2.2" and

Mid-infrared images between 8.7 and 18.7um of W75N were taken during three observing runs on September 2000, November 2001 and September 2003 with the mid-infrared camera CID on the 2.1 m telescope of the Observatorio Astronomico Nacional at San Pedro Martir, Baja California, Mexico. The images at 3.6, 4.5, 5.8 and 8.0um of W75N presented here are

Aims:We combine the magnetohydrodynamic (MHD) theory of resonantly damped quasi-mode kink oscillations with observational estimates of the period and damping of transverse coronal loop oscillations to extract information on physical parameters in oscillating loops. Methods: A numerical study of the quasi-mode period and damping, in one-dimensional