PPT-AGB stars in Galactic Globular Clusters –

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. brPage 1br Apian Globular II Pseudocylindrical Globular Neither Conformal or Equalarea Peter Apian or Bienewitz 1524 Apian Globular II Pseudocylindrical Globular Neither Conformal or brPage 1br Apian Globular I Pseudocylindrical Globular Neither Conformal or Equalarea Peter Apian or Bienewitz 1524 Apian Globular I Pseudocylindrical Globular Neither Conformal or Eq iPTF. Eric . Bellm. , . Frank . Masci. , Gandalf Saxe, . Sumin. Tang . [Tom Prince]. 27 Aug 2014. Galactic plane data is new. BEFORE. 2013 July 2nd. Galactic plane data is new. 2014 August 20th. AFTER. Hiroshi Imai. Graduate School of Science and Engineering, Kagoshima University. Contents. Astrometry with VLBA. , and VERA (EVN . for OH masers) . Results of astrometry. IRAS 19134+2131. K3-35. IRAS 19312+1950. 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. . Soprano I Hence  stars,  you  daz- zle but the sight,   you teach to Soprano II Hence  stars, \r \r \r Alto Hence  stars, hence   stars too  dim of light,  you  daz-  zle  b 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). 23.1 Our Parent Galaxy. 23.2 Measuring the Milky Way. Early “Computers”. 23.3 Galactic Structure. 23.4 The Formation of the Milky Way. 23.5 Galactic Spiral Arms. Density Waves. 23.6 The Mass of the Milky Way Galaxy. of . planetary nebulae, . jets and cosmic . outbursts. Orsola De . Marco. Macquarie University. Collaborators: . Jan Staff (Florida State). Jean-Claude Passy (Bonn U). Roberto Iaconi (Macquarie U). Todd . Chapter . 13, . Sections . 1. -5,7 (12 . pages). Homework for Next Time: . www.galaxyzoo.org. Question. Which of these is a picture of the Milky Way?. A. B. D. C. The Milky Way. Angular Size. Andromeda: MW’s Sister Galaxy. 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. 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. Maurizio . Spurio, . maurizio.spurio@unibo.it. . Università. di Bologna e INFN. 1. M. Spurio - Galactic template neutrino searches. Propagation induces accidents. M. Spurio - Galactic template neutrino searches. 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).