PPT-Formation of Globular Clusters in

Author : luanne-stotts | Published Date : 2016-04-28

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

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Formation of Globular Clusters in: Transcript


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 gasrich galaxies. brPage 1br Apian Globular II Pseudocylindrical Globular Neither Conformal or Equalarea Peter Apian or Bienewitz 1524 Apian Globular II Pseudocylindrical Globular Neither Conformal or Globular clusters are spherical collections of densely packed stars relics of the early years of the Universe with ages of typically 12 to 13 billion years This is very old considering that the Universe is only 138 billion years old Messier 22 is on 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. Are They Chemically Distinct to Their Fellow RGB and HB Stars?. M5: SDSS . Simon . Campbell. 1. . Universitat. . Politecnica. de . Catalunya. , Barcelona, Spain. 2. CSPA, . Monash. University, Melbourne, Australia. 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. . 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 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). 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 the Milky Way. Christian Johnson. Smithsonian Astrophysical Observatory. “Typical” Globular Clusters. Main Sequence. Main Sequence Turn-off. Subgiant Branch. Red Giant Branch. Horizontal Branch. Oleg . Gnedin. (University of Michigan. ). g. raduate student . Hui. Li. Star clusters are dominant components of active star formation:. they connect small-scale SF (local) and global processes in galaxies. 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 . Laura . Magrini. INAF- . Osservatorio. . Astrofisico. di . Arcetri. In Our Galaxy. Open clusters (disc population): . Many (~2200 known clusters). . even more new candidates in the inner disc from infrared surveys . 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). 1. Important. .. Extra Information.. Doctors slides. There is no elevator to success, you have to take the stairs !. 436 Biochemistry team. 2. Objectives:. describe the globular proteins using common examples like hemoglobin and myoglobin..

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