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Carroll & Ostlie, An Introduction to Modern Astrophysics Hilditch, An introduction to close binary stars Both on closed reserve in SciTech library. Lecture 1: Astrophysics Introduction 7 / 35. Astrophysics Astrophysics is a big subject. Sometimes will just flag where a whole (possibly large!) field branches

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Astrophysics Research Institute The Astrophysics Research Institute (ARI) is one of the world’s leading authorities in astronomy and astrophysics. Its work encompasses a comprehensive programme of observational and theoretical research, telescope operation, instrument development, academic learning and outreach activities. The ARI has been honoured with various awards and prizes including: n .

Astrophysics also receives tactical-level advice from the external science community via the Astrophysics Subcommittee of the NASA Advisory Council, and advice on cooperative activities from the Congressionally chartered, National Science Foundation (NSF)-managed Astronomy and Astrophysics Advisory Committee. NASA enables research to understand the structure, content, and evolution of the .

Astrophysics always offers a large range of M.Phys projects, from technical work in radio and optical astronomy through observational work with the Wetton telescope to numerical simulations, modelling and theory. We always ensure that every C1 student who wishes to do an astrophysics M.Phys. project is catered for. Astrophysics is a very sociable department! C1 students are encouraged to .

41 Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA 42 Universit e Paris-Saclay, CNRS . 5640 S. Ellis Ave., Chicago, IL 60637, USA 44 Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA 45 National Center for Supercomputing Applications (NCSA), University of Illinois .

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Astronomy, Astrophysics, and Cosmology Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson VII March 29, 2016 arXiv:0706.1988 L. A. Anchordoqui (CUNY) Astronomy, Astrophysics, and Cosmology 3-29-2016 1 / 22

CONTENTS Highlights 1 In a Nutshell 5 Textbooks 6 Princeton Frontiers in Physics 7 Biological Physics 8 Condensed Matter 9 Quantum Physics 9 Astronomy & Astrophysics 10 Princeton Series in Astrophysics 12 Princeton Series in Modern Observational Astronomy 13 Princeton Series in Physics 13 Mathematics, Mat

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Astrophysics needs input of practically all sub-disciplines of physics and thus a course on astrophysics cannot be self-contained. However, the course should be accessible to students with just a general introduction to physics. Few sections of the text that are somewhat more advanced and that can be omitted are marked by stars. I will be glad to receive feedback from the readers of these .

PARTICLE ASTROPHYSICS Dark Energy and Dark Matter 15 Dark energy There is a great deal of observational evidence from astrophysics and cosmology that the expansion of the universe is currently accelerating requires a component with equation of state P wƐwhere w 1/3 (w 1 is a vacuum energy or cosmological constant, Λ)

Laboratory astrophysics for stellar applications 221 the atomic data was, and in many cases, still is required. In this Talk and Proceedings Review paper we take stock of the achievements of Laboratory Astrophysics in terms of the advances made in the new atomic data now available to astronomers for iron group element neutral, singly and doubly ionised species, and also look to future data .

Longair: “High Energy Astrophysics” Rohlfs and Wilson: “Tools of Radio Astronomy” Dyson and Williams: “The Physics of the Interstellar Medium” Shu: “The Physics of Astrophysics I: Radiation” Radiation Processes We can measure the following quantities: The energy in the radiation as a function of a) position on the sky b) frequency The radiation’s .

Foundations of Astrophysics by Barbara Ryden and Bradley M. Peterson, a first course in astrophysics intended primarily for second-year majors in the physical sciences. SI units, augmented when necessary by various units peculiar to astronomy, are used throughout. In the written sol

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University of Chicago, Chicago, Illinois Richard. E. Emmert,* Wayne A. And.erson Laboratory for Astrophysics and. Space Research of the Enrico Fermi Institute for Nuclear Studies University of Chicago, Chicago, Illinois t James H. Patterson Chemistry Division Argonne National Laboratory, Argonne, Illinois and Ernest Franzgrote

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New Worlds, New Horizons in Astronomy and Astrophysics 4 Astro2010 Committee Roger Blandford, Chair, Stanford University Lynne Hillenbrand, Executive Officer, California Institute of Technology Subcommittee on Science Martha P. Haynes, Vice Chair - Science Frontiers, Cornell University Lars Bildsten, University of California, Santa Barbara John E. Carlstrom, The University of Chicago

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Gamma-ray Astrophysics Galaxy Evolution Observations of 'nearby' gamma-ray blazars have been used to place limits on the extragalactic background light (EBL) in the optical and IR. Aharonian et al., (2006) Nature 440, 1018 (z 0.186) MAGIC Collab., Science 320, 1752 (2008) (z 0.536) typical electron population

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