Matt Jarvis - Recent results from the Herschel-ATLAS
Riunione Avanzamento 1 ASI – Roma 11 Novembre 2008 INAF IFSI IRA OAFI OACT UNIRM1 UNIRM2 UNILE 1 SWG3: Evolution of Young Stellar Objects Goals Establish.
ExoZodiacal Emission and Challenge and Opportunity for The Detection of ExoPlanets C. Beichman Friday, March 26, 2010 5 AU Workshop With lots of help from.
A 100 parsec elliptical and twisted ring of cold and dense molecular clouds revealed by herschel around the galactic center
Dust production and_particle_acceleration_in_supernova_1987_a_revealed_with_alma
The first hyper_luminous_infrared_galaxy_discovered_by_wise
Big Questions If astronomers measure an object’s apparent brightness (flux), what do they need to know to figure out how far away that object is? Why are.
ASTR112 The Galaxy Lecture 7 Prof. John Hearnshaw 11. The galactic nucleus and central bulge 11.1 Infrared observations (cont.) 11.2 Radio observations.
Leaning objectives: Explain that: Elements as heavy as iron are formed inside stars by nuclear fusion. Heavier elements are formed in supernovas. Exploding.
The Interstellar Medium Chapter 10. You have begun your study of the sun and other stars, but now it is time to study the thin gas and dust that drifts.
SOFIA/HAWC polarimetry of low-mass YSOs and their environs.