'Galactic open clusters' diaporamas de présentation

The structure and evolution of stars

The structure and evolution of stars. Lecture 9: Computation of stellar evolutionary models. Learning Outcomes. The student will learn How to interpret the models of modern calculations - (in this case the models from the Geneva theoretical stellar evolution group)

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Current Status of Lulin Observatory and of the One-Meter Telescope: Operation and Management

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Gyrochronology in the Era of Wide-field, High-cadence, Synoptic Photometric Surveys

Gyrochronology in the Era of Wide-field, High-cadence, Synoptic Photometric Surveys. Establishing the Membership and Ages of Galactic Open Clusters. http://www.quantumdiaries.org/wp-content/uploads/2011/02/11-0035-08D1.jpg. VU KELT Meeting: Nashville, TN , 2011

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M ORPHOLOGY OF G ALACTIC O PEN C LUSTERS

Fig3: NGC1893. Fig.4: NGC1931. Fig.5 NGC2420. Fig6: Eccentricity vs. z of the 36 open clusters in our sample. Fig.7: Eccentricity vs. age of our sample clusters.

115 views • 1 slides