PPT-K2 Observations of Open Clusters

Ann Marie Cody NPP fellow at NASA Ames November 2 2015 Acknowledgments Ames collaborators Steve Howell Tom Barclay Fergal Mullally Susan Thompson Geert Barentsen Jason Rowe student interns Bryan Mann . the first 40 years, 1953-92 . What is a Blue Straggler?. “The Failure of Occam’s Razor?” . . (Mario . Livio. 1993, ASP Conf. 53, ed. R . Saffer. , p.3). Why has it taken so long?. Inconclusive and confusing early observations. Michael E. Goodrich & David T. Moore. Chemistry Department, Lehigh University. Bethlehem PA, 18015. 1. Introduction. CO Oxidation on metal center. Cu(CO). m. (O. 2. ). n . complexes difficult to form. in Solar Disk Images . (and how to compare to models). Working Group Report. Nick Arge. .  . Rachel Hock. .  . Carl Henney. Definitions . (from our invited speakers). Coronal holes. : observable used as. With a wide-field multi-IFU spectrograph. Cluster studies. Clusters provide large samples of galaxies in a moderate field. Unique perspective on the interaction of galaxies with their environment. As they operate much as a closed box, they are useful as tracers of galaxy evolution and of cosmology. . CDM Cosmology. Oleg . Gnedin. (University of Michigan. ). What we knew before HST: globular clusters are old, dense, compact – a distinct type of stellar spheroids. Kormendy. (1985). Over 20 years the Hubble Space Telescope has revealed young massive star clusters in interacting and gas-rich galaxies.. Stat 600. Nonlinear DA. We discussed LDA where our . discriminant. boundary was linear. Now, lets consider scenarios where it could be non-linear. We will discuss:. QDA. RDA. MDA. As before all these methods aim to MINIMIZE the probability of misclassification.. Essay: Globular and Open Clusters - Course: HET 603, September 2002Instructor: Dr. Chris Flynn - Student: Eduardo Manuel Alvarezattraction. Being so far as they are, all the stars belonging to the s The Milky Way: Our Home Galaxy. What are the different. components of the Milky Way?. How do we see those components?. What does a map of each component look like from our point of view?. Stars in the Milky Way. in collaboration with. Christine Jones & Bill Forman. Maxim Markevitch & John Zuhone. A . talk . for the . workshop “Diffuse . Emission from Galaxy Clusters in the Chandra . Era”. . by. Ryan E. Johnson. Wen-Ping . Chen . National . Central . University . Census of Galactic open clusters. . Dynamical evolution of a star cluster. . Star clusters as targets and as tools. Outstanding issues. 2017 April 28 PMO . CMIS Short Course part II. Day 1 Part 1:. Clustering. Sam Buttrey. December 2015. Clustering. Techniques for finding structure in a set of measurements. Group X’s without knowing their y’s. Usually we don’t know number of clusters. Fornax and Virgo Clusters Gas Dynamics Merger History and Elemental EnrichmentR Kraft1Y Su1T Fish21A Sheardown2E Roediger21W Forman1C Jones1P Nulsen1E Churazov3 S Randall1 EBulbul11Smithsonian Astrop Valid Open-E High Availability Certified Storage Clusters Practice Course


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