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The top documents tagged [warm dust]
Matt Jarvis - Recent results from the Herschel-ATLAS
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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
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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
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A 100 parsec elliptical and twisted ring of cold and dense molecular clouds revealed by herschel around the galactic center
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Dust production and_particle_acceleration_in_supernova_1987_a_revealed_with_alma
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The first hyper_luminous_infrared_galaxy_discovered_by_wise
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The first hyper_luminous_infrared_galaxy_discovered_by_wise
4.566 views
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
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ASTR112 The Galaxy Lecture 7 Prof. John Hearnshaw 11. The galactic nucleus and central bulge 11.1 Infrared observations (cont.) 11.2 Radio observations
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Leaning objectives: Explain that: Elements as heavy as iron are formed inside stars by nuclear fusion. Heavier elements are formed in supernovas. Exploding
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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
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SOFIA/HAWC polarimetry of low-mass YSOs and their environs
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