Galaxies in the Local Volume

Editors:

ISBN: 978-1-4020-6932-1 (Print) 978-1-4020-6933-8 (Online)

Table of contents (102 chapters)

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  1. Front Matter

    Pages 1-18

  2. Invited and Contributed Talks

    1. Front Matter

      Pages 1-1

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      Book Chapter

      Pages 3-12

      The Local Velocity Anomaly

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      Book Chapter

      Pages 13-16

      Outlining the Local Void with the Parkes HI ZOA and Galactic Bulge Surveys

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      Book Chapter

      Pages 17-20

      The Context of the Local Volume: Structures and Motions in the Nearby Universe

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      Book Chapter

      Pages 21-30

      Mining the Local Volume

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      Pages 31-36

      Properties of Voids in the Local Volume

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      Book Chapter

      Pages 37-40

      Using Local Volume Data to Constrain Dark Matter Dynamics

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      Pages 41-44

      The Local Volume HI Survey (LVHIS)

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      Book Chapter

      Pages 45-48

      Investigating Dark Matter and MOND in Local Volume Galaxies

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      Book Chapter

      Pages 49-52

      Deepest Near-IR Surface Photometry of Galaxies in the Local Sphere of Influence

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      Book Chapter

      Pages 53-56

      Ionized and Neutral Gas in the Starburst Galaxy NGC 5253

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      Pages 57-60

      The Smallest HI Galaxies

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      Pages 61-64

      FIGGS Faint Irregular Galaxies GMRT Survey

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      Pages 65-68

      Gas Rich Galaxies from the FIGGS Survey

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      Pages 69-72

      The Evolution of the ISM in Star Forming Galaxies

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      Pages 73-76

      Magnetic Fields in Irregular Galaxies

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      Pages 77-80

      Future ASKAP Studies of the Local Volume

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      Book Chapter

      Pages 81-84

      An Ultraviolet-to-Radio Broadband Spectral Atlas of Nearby Galaxies

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      Book Chapter

      Pages 85-88

      Diagnostic Value of Mid-Infrared Fine Structure Lines in Galaxies

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      Book Chapter

      Pages 89-92

      Warm Molecular Hydrogen in Nearby Galaxies Results from the SINGS Sample

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      Book Chapter

      Pages 93-96

      Molecular Gas Cloud Properties and Star Formation in Dwarf Galaxies

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