Disks around young Brown Dwarfs as critical testbeds for models of dust evolution: an investigation with ALMA Luca Ricci (CARMA Fellow, Caltech) Testi.
Far ultraviolet morphology_of_star_forming_filaments_in_cool_core_brighest_cluster_galaxies
Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen Liske European Southern Observatory Frank Briggs Australian.
The SED of the nearby, HI-massive, LIRG HIZOA J0836-43: from the NIR to the radio domain Renée C. Kraan-Korteweg Astronomy Department Centre for Astrophysics.
X-ray view of the most obscured QSOs at high redshift Chiara Feruglio CNRS - CEA, Saclay
VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties in arm and interarm regions. Higher densities and stronger.
Direct Physical Diagnostics of Triggered Star Formation Rachel Friesen NRAO Postdoctoral Fellow North American ALMA Science Center C. Brogan, R. Indebetouw,
Mapping HI absorption at z=0.026 against a resolved background CSO
VNGS science highlight: PDR models of M51
The SED of the nearby, HI-massive, LIRG HIZOA J0836-43: from the NIR to the radio domain
Disks around y oung Brown Dwarfs as critical testbeds for