The top documents tagged [ms stars]

Everything you always wanted to know about stars… Material from Chapters 8 and 9 in Horizons by Seeds 0
Documents Everything you always wanted to know about stars… Material from Chapters 8 and 9 in Horizons by Seeds 0

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1/9/2003Ringberg Workshop1 Recent science results from VLTI commissioning Francesco Paresce European Southern Observatory
Documents 1/9/2003Ringberg Workshop1 Recent science results from VLTI commissioning Francesco Paresce European Southern Observatory

218 views

T Tauri Stars Kate Barnes A540. T Tauri Stars: Background Very young, solar-type stars ~10 7 yrs Low mass 0.5 M < M < 2 M Name: T Tauri, found in Taurus-Auriga
Documents T Tauri Stars Kate Barnes A540. T Tauri Stars: Background Very young, solar-type stars ~10 7 yrs Low mass 0.5 M < M < 2 M Name: T Tauri, found in Taurus-Auriga

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O. Absil & C. Eiroa with inputs from A. Roberge, D. Defrère, C. Beichman, W. Danchi, J.-C. Augereau, etc. O. Absil & C. Eiroa with inputs from A. Roberge,
Documents O. Absil & C. Eiroa with inputs from A. Roberge, D. Defrère, C. Beichman, W. Danchi, J.-C. Augereau, etc. O. Absil & C. Eiroa with inputs from A. Roberge,

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Christian Knigge University of Southampton School of Physics & Astronoy Cataclysmic Variables: 10 Breakthroughs in 10 Years P. Marenfeld and NOAO/AURA/NSF
Documents Christian Knigge University of Southampton School of Physics & Astronoy Cataclysmic Variables: 10 Breakthroughs in 10 Years P. Marenfeld and NOAO/AURA/NSF

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SPECTROSCOPY OVERVIEW The Science Case: High Resolution Spectroscopy of (cool) stars Basic tools for specifications and verification One example of similar
Documents SPECTROSCOPY OVERVIEW The Science Case: High Resolution Spectroscopy of (cool) stars Basic tools for specifications and verification One example of similar

217 views

1 Some key problems and key reactions in Nuclear Astrophysics Main issues: BBN: was the universe always the same? What’s in the core of Sun and other MS
Documents 1 Some key problems and key reactions in Nuclear Astrophysics Main issues: BBN: was the universe always the same? What’s in the core of Sun and other MS

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The Effects of Mass Loss on the Evolution of Chemical Abundances in Fm Stars Mathieu Vick 1,2 Georges Michaud 1 (1)Département de physique, Université
Documents The Effects of Mass Loss on the Evolution of Chemical Abundances in Fm Stars Mathieu Vick 1,2 Georges Michaud 1 (1)Département de physique, Université

217 views

The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different
Documents The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different

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Improving our understanding of Stellar Evolution with PLATO 2.0 Santi Cassisi INAF - Astronomical Observatory of Teramo, Italy
Documents Improving our understanding of Stellar Evolution with PLATO 2.0 Santi Cassisi INAF - Astronomical Observatory of Teramo, Italy

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WFC3/IR LESSONS FOR WFIRST Jay Anderson STScI. WFC3/IR Lessons for WFIRST 1)Absolute astrometry 2)PSF modeling and variation (space/time) 3) Bulge-type
Documents WFC3/IR LESSONS FOR WFIRST Jay Anderson STScI. WFC3/IR Lessons for WFIRST 1)Absolute astrometry 2)PSF modeling and variation (space/time) 3) Bulge-type

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Star Clusters
Documents Star Clusters

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