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The top documents tagged [warm dust]
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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
4.567 views
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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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.
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