'Dust properties' diaporamas de présentation

Cumber01 30.5.2001

Thomas Henning Max Planck Institute for Astronomy, Heidelberg. _______________. The Lifecycle of Dust in the Universe From Alpha to Omega. M 31 with Herschel/PACS (70 + 160 ? m) + SPIRE (250 ? m) (Groves et al. 12; Smith et al. 12, Krause et al. 14; Dust: Draine et al. 13)

492 views • 35 slides

Dust Properties Retrieved from the AERI Observations at Niamey

Dust Properties Retrieved from the AERI Observations at Niamey. Dave Turner Space Science and Engineering Center University of Wisconsin - Madison. Overview. Atmospheric Emitted Radiance Interferometer General description of instrument Calibration approach Data corrections needed

376 views • 26 slides

Scattered light images of protoplanetary and debris disks

313 views • 19 slides

Francesco Trotta

Using mm observations to constrain variations of dust properties in circumstellar disks. Francesco Trotta. Advised by: Leonardo Testi. YERAC, Manchester - 2011. Outline. Planet Formation in circumstellar disks Observational evidence of dust grain growth

294 views • 18 slides

FarIR Properties of Submm and Optically-Faint Radio Galaxies using Herschel

FarIR Properties of Submm and Optically-Faint Radio Galaxies using Herschel. Scott C. Chapman (IoA ,Cambridge) Rob Ivison (ROE,ATC), Isaac Roseboom & Seb Oliver (Sussex) SAG1-HerMES team. July6 2010, Cumberland Lodge. OUTLINE. ~1000M/yr SFR at z>1 ? ULIRG/HyLIRG

312 views • 18 slides

The Impact of Dust on a Stellar Wind-Blown Bubbles

Ed Churchwell & John Everett University of Wisconsin Oct. 12-15, 2008 Lowell Observatory Flagstaff, AZ. The Impact of Dust on a Stellar Wind-Blown Bubbles. Outline N49-A Stellar Wind-Blown Bubble. Dust observed within this wind-blown bubble MIR/Radio Image

284 views • 17 slides

Improving the Mars Thermal 1D Model

E. Millour, A Colaitis, F. Forget EXM-AMSA PM6, 7th July 2011. Improving the Mars Thermal 1D Model. Overview of the lmd1d tool. Initially provided by LMD to ESA in Feb. 2008 A simple, straightforward program designed to compute: - The downward thermal IR flux at the surface.

252 views • 16 slides

Improving the Mars Thermal 1D Model

E. Millour, A Colaitis, F. Forget EXM-AMSA PM6, 7th July 2011. Improving the Mars Thermal 1D Model. Overview of the lmd1d tool. Initially provided by LMD to ESA in Feb. 2008 A simple, straightforward program designed to compute: - The downward thermal IR flux at the surface.

163 views • 16 slides