PPT-The Globular Cluster-Galaxy Connection
Author : morton | Published Date : 2024-02-09
1 st meeting July 1992 Globular Clusters Within the Context of Their Parent Galaxies 2 nd meeting July 2011 KraftFest 2011 3 rd meeting July 2030 subtitle to be
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The Globular Cluster-Galaxy Connection: Transcript
1 st meeting July 1992 Globular Clusters Within the Context of Their Parent Galaxies 2 nd meeting July 2011 KraftFest 2011 3 rd meeting July 2030 subtitle to be decided at a later date. Globular Cluster M80 (Resolved by Galileo). Milky Way:. Galactic Structure and Dynamics. Milky Way has spiral structure. . Galactic Bulge surrounds the Center. . Powerful radio source Sagittarius A at Center. C. ontains Super-Massive Black Hole . Anja. von . der. Linden et al., 2007, MNRAS, 379, 867. On the prevalence of radio-loud active galactic nuclei in brightest cluster galaxies: implications for AGN heating of cooling flows. P. N. Best et al., 2007, MNRAS, 379, 894. . 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.. William Herschel’s map of the Milky Way based on star counts. In the early 1800’s William Herschel, the man who discovered the planet Uranus, tried to understand the shape of the Milky Way by counting stars. He counted how many stars there were in each of dozens of different directions and then plotted the count versus direction. . . Chris Haines . (Universidad de Chile). Paula . Merluzzi. , Gianni . Busarello. , . Amata. . Mercurio. . (Naples). , . Nobuhiro. Okabe . (IPMU). , Luis . Campusano. . (. U.Chile. ). ESO: Dissecting Galaxies Near and Far, 26th March 2015. Raffaele . Gratton. INAF – . Osservatorio. . Astronomico. di . Padova. , ITALY. Contribution to GC science: numbers. 139 entries in ADS with "Cohen, J." AND "globular“:. oldest 1975, most recent 2016 (query on Jan. 11, 2017). Outer Envelope Structure In Massive Globular Clusters. Pete Kuzma . PhD student, Research School of Astronomy and Astrophysics. Simulation of a tidally disrupted dwarf galaxy (K. . Johnston 2014). Field Of Streams. Naviance. , a . web based . service designed especially for students and parents. Family Connection is a comprehensive website that you and your child can use to help in making decisions about courses, colleges, and careers. Family Connection is linked with . A Research Project by Dominic Elizondo. Contrasting Open and Globular Clusters. Age. Location. Number of Stars. M2 Globular Cluster. M11 Open Cluster. Data Collection. 20’’ f/6.8 Plane Wave . Cassegrain. Here’s the mystery story we’ll unfold…. Fuzzy blobs in the sky – new solar systems, or “galaxies”?. Observational tests. Herschel’s map of the “universe” . (what we today know as just our Galaxy). Patrick L. Kelly et al. 2014 arXiv:1411.6009 . submitted to Nature. Summarised. . by Poonam Chandra. February 18, 2015. Poonam Chandra. 1. Punch line. Discovery of the . first multiply-imaged . gravitationally-lensed supernova.. Kelsey McCabe. University of Arizona. Advisor: Dennis . Zaritsky. . Department of Astronomy. University of Arizona. Arizona Space Grant . Symposium. Arizona State University. Tempe. , AZ. Outline. A Brief Overview. GUViCS. ). IV. The role of the cluster environment on galaxy evolution. Speaker: Xinkai Chen. Sample. Sample:. Extended Source . Catalogue of Voyer+14. recessional . velocity < . 3500kms-1. , Virgo cluster region.
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