A Multi-Scale Analysis of Magnetic Fields in Filamentary Molecular Clouds and Their Environments
We use visible and submm polarimetric data to trace, study and compare magnetic fields within and near elongated molecular clouds. A preliminary polarimetric...
We present preliminary results from a multisite photometric campaign on the intermediate polar V709 Cas carried out between Sept. 22 and Oct. 2, 2000. The...
A multi-wavelength approach to the properties of Extremely Red Galaxy populations: star formation rate and mass densities, AGN and dust content, and morphology
A Multi-Wavelength Study of Magnetic Activity in Praesepe and Hyades
Hyades and Praesepe are the oldest (≈700 Myr old) open clusters within 250 pc, and thus the oldest easily accessible ensembles of low-mass stars with a...
A Multi-wavelength Study of Rotation and Magnetic Activity in Young Open Clusters
In main-sequence, low-mass (<1.3 Solar mass) stars, rotation and magnetic activity decrease over time, with the spin-down thought to be due to angular momentum...
A multi-wavelength view of AGN feedback in the central kiloparsecs of quasar host galaxies
Active galactic nuclei (AGN) winds and jets are potential drivers of multi-phase outflows and can significantly modify the interstellar medium (ISM) properties...