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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
Everything you always wanted to know about stars… Material from Chapters 8 and 9 in Horizons by Seeds 0
214 views
1/9/2003Ringberg Workshop1 Recent science results from VLTI commissioning Francesco Paresce European Southern Observatory
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
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
216 views
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,
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,
221 views
Christian Knigge University of Southampton School of Physics & Astronoy Cataclysmic Variables: 10 Breakthroughs in 10 Years P. Marenfeld and NOAO/AURA/NSF
Christian Knigge University of Southampton School of Physics & Astronoy Cataclysmic Variables: 10 Breakthroughs in 10 Years P. Marenfeld and NOAO/AURA/NSF
223 views
SPECTROSCOPY OVERVIEW The Science Case: High Resolution Spectroscopy of (cool) stars Basic tools for specifications and verification One example of similar
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
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
214 views
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
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
The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different
218 views
Improving our understanding of Stellar Evolution with PLATO 2.0 Santi Cassisi INAF - Astronomical Observatory of Teramo, Italy
Improving our understanding of Stellar Evolution with PLATO 2.0 Santi Cassisi INAF - Astronomical Observatory of Teramo, Italy
218 views
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
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
212 views
Star Clusters
Star Clusters
43 views