On the Lack of Stellar Bars in Coma Dwarf Galaxies
We present a study of the bar fraction in the Coma cluster galaxies based on a sample of ~190 galaxies selected from the SDSS-DR6 and observed with the Hubble...
Using the Nordic Optical Telescope, La Palma, Spain, optical studies of OT/GRB970508 were initiated 3 hours 5 minutes after the high energy event (This appears...
On the Light-Profiles of Spiral Galaxy Bulges and the Hubble Sequence for Spirals
Recent studies have claimed that the Hubble sequence of late-type spirals, and spirals in general, is scale-free. Within the photometric data used in these...
On the Limits of Seismic Inversions for Radial Differential Rotation of Solar-Type Stars
Seismic data contains information on stellar internal rotation, which plays an important role on dynamo models. Due to the uncertainties on the observations and...
On The Magnetic-Field Diagnostics Potential of SDO/HMI
The Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) is designed to study oscillations and the magnetic field in the solar...
On the making of a PN: the interaction of a multiple stellar wind with the ISM
NGC 7293, the Helix nebula, represents one of the rare instances in which theoretical predictions of stellar evolution can be accurately tested against...
On the MG 2 and Fe 2 resonance lines in Herbig AE stars: Preliminary results
The IUE observed AB Aur, HD250550, and BD + 46 deg 3471 at high resolution in the range 2000 to 32000 A. The MgII resonance line profiles all show a P Cygni...
On the Nature of Damped LYα Systems: Clues from Determinations of Elemental Abundance Ratios
We present a study of the [α/Fe-peak] and [N/α] abundance ratios in Damped Lyα (DLA) systems. By using ratios of undepleted elements ([S/Zn] and [N/S]) or when...