Slide 1 SOFIA/HAWC polarimetry of low-mass YSOs and their environs Slide 2 SHARP Slide 3 SOFIA/HAWC polarimetry of low-mass YSOs and their environs SHARP Class 0 Slide 4…
Slide 1 Submillimeter Astronomy in the era of the SMA, Cambridge, June 14, 2005 Star Formation and Protostars at High Angular Resolution with the SMA Jes Jørgensen (CfA)…
Slide 1 + Current efforts for modeling exozodiacal disks Jean-Charles Augereau & Olivier Absil LAOG, Grenoble, France & U. Liège, Belgium Barcelona, September 2009…
ESO Galaxy Formation: The Radio Decade (Dense Gas History of the Universe) Chris Carilli (NRAO) Santa Fe, March 2011 Power of radio astronomy: dust, cool gas, and star formation…
INTEGRAL obscured sources and SFXTs INTEGRAL sources 499 point sources (20kev-100kev) 147XRBs, 163AGNs, 27CVs, 20 sources of other type: 12 SNs, 2 globular clusters, 2 SGRs…
ALMA ES capabilities: Distant Galaxies Alexandra Pope (UMass Amherst) JWST Workshop – STScI Baltimore June 8, 2011 Mid-Infrared Observation of High Redshift Galaxy Evolution…
The HST image shows a wealth of detail but what is it? Other edge-on spirals don’t look like M82. M83 is a scaled down face-on M82. M83 - H Similar to M82, there is…
VLASS – Galactic Science VLASS – Galactic Science Life cycle of star formation in our Galaxy as a proxy for understanding the Local Universe legacy science Infrared GLIMPSE…
Leaning objectives: Explain that: ⢠Elements as heavy as iron are formed inside stars by nuclear fusion. ⢠Heavier elements are formed in supernovas. ⢠Exploding…
Great Observatories Galactic Center Region Image Unveiling Science Telecon October 6, 2009 Multiwavelength Observations Dr. Frank Summers Support Web Site http://hubblesource.stsci.edu/events/iyafinale/support/…