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Disks around young Brown Dwarfs as critical testbeds for models of dust evolution: an investigation with ALMA Luca Ricci (CARMA Fellow, Caltech) Testi.
Documents Disks around young Brown Dwarfs as critical testbeds for models of dust evolution: an investigation....

Slide 1Disks around young Brown Dwarfs as critical testbeds for models of dust evolution: an investigation with ALMA Luca Ricci (CARMA Fellow, Caltech) Testi (ESO/Arcetri),…

Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen Liske European Southern Observatory Frank Briggs Australian.
Documents Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen....

Slide 1 Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen Liske European Southern Observatory Frank Briggs Australian National…

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.
Documents The SED of the nearby, HI-massive, LIRG HIZOA J0836-43: from the NIR to the radio domain Renée C......

Slide 1 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 Cosmology…

X-ray view of the most obscured QSOs at high redshift Chiara Feruglio CNRS - CEA, Saclay
Documents X-ray view of the most obscured QSOs at high redshift Chiara Feruglio CNRS - CEA, Saclay

X-ray view of the most obscured QSOs at high redshift Chiara Feruglio CNRS - CEA, Saclay IRAM - Institut de RadioAstronomie Millimetrique  thanks to: Daddi, Fiore, Piconcelli,…

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.
Documents VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties.....

VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/FTIR Similar gas properties in arm and interarm regions. Higher densities and stronger radiation fields…

Direct Physical Diagnostics of Triggered Star Formation Rachel Friesen NRAO Postdoctoral Fellow North American ALMA Science Center C. Brogan, R. Indebetouw,
Documents Direct Physical Diagnostics of Triggered Star Formation Rachel Friesen NRAO Postdoctoral Fellow...

Slide 1 Direct Physical Diagnostics of Triggered Star Formation Rachel Friesen NRAO Postdoctoral Fellow North American ALMA Science Center C. Brogan, R. Indebetouw, C. Cyganowski,…

The SED of the nearby, HI-massive, LIRG HIZOA J0836-43: from the NIR to the radio domain
Documents The SED of the nearby, HI-massive, LIRG HIZOA J0836-43: from the NIR to the radio domain

Unveiling HIZOAJ0836-43 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…

Disks around y oung Brown Dwarfs as critical testbeds for
Documents Disks around y oung Brown Dwarfs as critical testbeds for

Testing the models of early evolution of solids in disks through sub-mm interferometry Disks around young Brown Dwarfs as critical testbeds for models of dust evolution:…

Far ultraviolet morphology_of_star_forming_filaments_in_cool_core_brighest_cluster_galaxies
Science Far ultraviolet morphology_of_star_forming_filaments_in_cool_core_brighest_cluster_galaxies

1. MNRAS 451, 3768–3800 (2015) doi:10.1093/mnras/stv1151 Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies G. R. Tremblay,1,2‹…

Mapping HI absorption at z=0.026 against a resolved background CSO
Documents Mapping HI absorption at z=0.026 against a resolved background CSO

First full-field image Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen Liske European Southern Observatory Frank Briggs…

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