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The top documents tagged [massive stars]

Current Topics: Lyman Break Galaxies - Elizabeth Stanway 1 Current Topics Lyman Break Galaxies Dr Elizabeth Stanway (E.R.Stanway@Bristol.ac.uk)
Current Topics: Lyman Break Galaxies - Elizabeth Stanway 1 Current Topics Lyman Break Galaxies Dr Elizabeth Stanway ([email protected])
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Strategic Exploration of Exoplanets and Disks with Subaru: SEEDS Nobuhiko Kusakabe, Motohide Tamura, Ryo Kandori, Tomoyuki Kudo, Jun Hashimoto, SEEDS/HiCIAO/AO188
Strategic Exploration of Exoplanets and Disks with Subaru: SEEDS Nobuhiko Kusakabe, Motohide Tamura, Ryo Kandori, Tomoyuki Kudo, Jun Hashimoto, SEEDS/HiCIAO/AO188
213 views
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,
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,
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E. Pian – LNGS, 13 Sep 2005 Elena Pian - INAF, Trieste Astronomical Observatory, Italy LNGS Summer Institute 2005 GRB: Modern Status
E. Pian – LNGS, 13 Sep 2005 Elena Pian - INAF, Trieste Astronomical Observatory, Italy LNGS Summer Institute 2005 GRB: Modern Status
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Where might we find life in the Solar System? Temperatures of planets
Where might we find life in the Solar System? Temperatures of planets
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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
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
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UV radiative feedbackRingberg, Germany 24-27. march, 2009 UV Radiative Feedback During Reionization Andrei Mesinger Princeton University
UV radiative feedbackRingberg, Germany 24-27. march, 2009 UV Radiative Feedback During Reionization Andrei Mesinger Princeton University
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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
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
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
Course evaluations. Go to the Physics and Astronomy Department website. Click on Online Course Evaluation link Link is open now. Do it
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The VLTI view of compact dusty environments around evolved stars Olivier CHESNEAU Observatoire de la Côte dAzur (OCA)
The VLTI view of compact dusty environments around evolved stars Olivier CHESNEAU Observatoire de la Côte dAzur (OCA)
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Electromagnetic Spectrum. Electromagnetic energy travels in waves and spans a broad spectrum from very long radio waves to very short gamma rays. Our
Electromagnetic Spectrum. Electromagnetic energy travels in waves and spans a broad spectrum from very long radio waves to very short gamma rays. Our
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