Slide 1 Galaxies-I Slide 2 By the 1700’s the old notion that the Earth was the center of the Universe was overthrown by the success of Newton’s theory of universal gravitation,…
Slide 1The Science behind the Eagle Nebula Image Howard E. Bond Space Telescope Science Institute and Co-founder, Hubble Heritage Team Slide 2 Dust pillar in the Eagle Nebula,…
Slide 1 Slide 2 OPEN STAR CLUSTER M11 Rosalina Bonilla Jennifer Hsieh Mary Lou Juanatas Cluster 7: Stars, Sight, and Science Slide 3 OUTLINE Background of Star Clusters Background…
Slide 1 Two Sightlines toward the Galactic Center with Remarkable H 3 + and CO Spectra Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry, The…
Slide 1 Distances Slide 2 Parallax Near objects appear to move more than far objects against a distant horizon. Trigonometric parallax is used to measure distance to near…
Slide 1 2 vi 2006Bethe Centenary Cornell1 The Future of High Energy Astrophysics Extreme Physics in an Expanding Universe Roger Blandford KIPAC Stanford Hans Bethe Centenary,…
Les Pulsars gamma avec GLAST David Smith Centre d’Etudes Nucléaires de Bordeaux-Gradignan ( CENBG - in2p3 - CNRS ) Moriond 4 February 2009 GeV Galactic Sources with the…
H3+ Search for hot and bright stars for H3+ spectroscopy Near the Galactic center Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry The Enrico…
Galaxies GALAXY - comes from the ancient Greeks and their word for âmilkâ-galactos GALAXY are large systems of stars and interstellar matter typically containing several…
Galaxies â Island Universes Hereâs the Story Weâll Unfold for You⦠Hubbleâs galaxy classifications: Spirals, ellipticals, irregulars. Structural parts of galaxies:…