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The top documents tagged [massive stars]
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massive stars
Strategic Exploration of Exoplanets and Disks with Subaru: SEEDS Nobuhiko Kusakabe, Motohide Tamura, Ryo Kandori, Tomoyuki Kudo, Jun Hashimoto, SEEDS/HiCIAO/AO188.
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The Quest for Massive Protostars Sergio Molinari IFSI-CNR, Roma S. Pezzuto, L. Montinaro @ IFSI-CNR, Roma L. Testi, R. Cesaroni, F. Palla, F. Fontani,
230 views
E. Pian – LNGS, 13 Sep 2005 Elena Pian - INAF, Trieste Astronomical Observatory, Italy LNGS Summer Institute 2005 GRB: Modern Status.
218 views
Where might we find life in the Solar System? Temperatures of planets.
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UV radiative feedbackRingberg, Germany 24-27. march, 2009 UV Radiative Feedback During Reionization Andrei Mesinger Princeton University.
216 views
Xavier Barcons Instituto de Física de Cantabria (CSIC-UC) On behalf of The Athena+ Co-ordination Group, the Athena+ Working Groups and Supporters A theme.
214 views
1 To Be or Not to Be: The Mysteries of Disk Formation Around Rapidly Spinning Be Stars Douglas R. Gies Department of Physics and Astronomy Center for High.
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Accretion Disks around Stars and the Process of Planet Formation National Radio Astronomy Observatory The National Radio Astronomy Observatory is a facility.
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Course evaluations. Go to the Physics and Astronomy Department website. Click on Online Course Evaluation link Link is open now. Do it.
212 views
Electromagnetic Spectrum. Electromagnetic energy travels in waves and spans a broad spectrum from very long radio waves to very short gamma rays. Our.
230 views
Star Formation Why is the sunset red? The stuff between the stars Nebulae Giant molecular clouds Gravitational collapse of molecular cloud Gravitational.
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The Formation and Structure of Stars Chapter 9. The Big Picture Stars exist because of gravity. Gravity causes interstellar material to collapse to form.
226 views
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