Penetrating Bars through Masks of Cosmic Dust The Hubble Tuning Fork strikes a New Note

THE EDITORS: DAVID L. BLOCK AND KENNETH C. FREEMAN (SOC CO-CHAIRS), IVANIO PUERARI, ROBERT GROESS AND LIZ K. BLOCK 1. Harvard College Observatory, 1958 The past century has truly brought about an explosive period of growth and discovery for the physical sciences as a whole, and for astronomy in part...

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Bibliographic Details
Other Authors: Block, David L. (Editor), Puerari, Ivânio (Editor), Freeman, K. C. (Editor), Groess, R. (Editor)
Format: eBook
Language:English
Published: Dordrecht Springer Netherlands 2004, 2004
Edition:1st ed. 2004
Series:Astrophysics and Space Science Library
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
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245 0 0 |a Penetrating Bars through Masks of Cosmic Dust  |h Elektronische Ressource  |b The Hubble Tuning Fork strikes a New Note  |c edited by David L. Block, Ivânio Puerari, K. C. Freeman, R. Groess, Elizabeth K. Block 
250 |a 1st ed. 2004 
260 |a Dordrecht  |b Springer Netherlands  |c 2004, 2004 
300 |a XXIII, 881 p  |b online resource 
505 0 |a The Editors – Preface -- A Tribute to Cosmic Dust Pioneer J. Mayo Greenberg -- The Hubble Tuning Fork Strikes a New Note -- Episodes in the Development of the Hubble Galaxy Classification -- Secular Evolution Versus Hierarchical Merging: Galaxy Evolution along the Hubble-sequence, in the Fields and Rich Environments -- Dense Gas and Star Formation in Bars -- On the Origin of S0 Galaxies -- Gravitational Bar Torques in the Spiral/S0 Divide -- Direct Measurement of Pattern Speeds In Double-Barred SB0's -- Gas Flows, Star Formation and Galaxy Evolution -- Bar-Driven Evolution and 2D Spectroscopy of Bulges -- Bar-Driven Fueling of Galactic Nuclei: a 2D view -- Dust Penetrated Arm Classes: Insight form Rising and Falling Rotation Curves -- Bar Dissolution and Reformation Mechanisms -- Dynamics of Doubly Barred Galaxies, also with the Inner Bar Retrograde -- A Coordinated Episode of AGB Star Production at Large Galactocentric Distances in the Andromeda Galaxy --  
505 0 |a Bar-Driven Evolution and 2D Spectroscopy of Bulges -- Bar-Driven Fueling of Galactic Nuclei: a 2D view -- Dust Penetrated Arm Classes: Insight form Rising and Falling RotationCurves -- Bar Dissolution and Reformation Mechanisms -- Dynamics of Doubly Barred Galaxies, also with the Inner Bar Retrograde -- A Coordinated Episode of AGB Star Production at Large Galactocentric Distances in the Andromeda Galaxy -- Fuelling Starbursts and AGN -- Penetrating Dust Tori in AGN -- Bars from the Inside Out: An HST Study of their Dusty Circumnuclear Regions -- Morphology of Bar and Spiral Modes: do they relate?- Bar Formation by Galaxy-Galaxy Interactions -- Triggering AGNs - Interactions or Bars?- Triggered Star Formation: from Large to Small Scales -- Investigation of Age and Metallicity Gradients in Spiral Galaxies -- Secular Evolution and the Growth of Pseudobulges in Disk Galaxies -- Bars and Lences in Spiral Galaxies: Clues for Secular Evolution --  
505 0 |a High Resolution Velocity Fields in the Strongly Barred Galaxy NGC 1530 -- Panel Discussion -Closing Conference Thoughts.-The Noblest Scientific Problem of the Age: Perspectives on the Transit of Venus, 1882 and 2004 Description of the Commemorative Medallion, Struck to Celebrate the Transition of Venus, Observed from South Africa on 8 June 2004 -- Caption for Colour plates -- The 16 colour plates -- List of Participants. The Editors – Preface -- A Tribute to Cosmic Dust Pioneer J. Mayo Greenberg -- The Hubble Tuning Fork Strikes a New Note -- Episodes in the Development of the Hubble Galaxy Classification -- Secular Evolution Versus Hierarchical Merging: Galaxy Evolution along the Hubble-sequence, in the Fields and Rich Environments -- Dense Gas and Star Formation in Bars -- On the Origin of S0 Galaxies -- Gravitational Bar Torques in the Spiral/S0 Divide -- Direct Measurement of Pattern Speeds In Double-Barred SB0s -- Gas Flows, Star Formation and Galaxy Evolution --  
505 0 |a Fuelling Starbursts and AGN -- Penetrating Dust Tori in AGN -- Bars from the Inside Out: An HST Study of their Dusty Circumnuclear Regions -- Morphology of Bar and Spiral Modes: do they relate?- Bar Formation by Galaxy-Galaxy Interactions -- Triggering AGN's - Interactions or Bars?- Triggered Star Formation: from Large to Small Scales -- Investigation of Age and Metallicity Gradients in Spiral Galaxies -- Secular Evolution and the Growth of Pseudobulges in Disk Galaxies -- Bars and Lences in Spiral Galaxies: Clues for Secular Evolution -- Evolution and Impact of Bars over the last nine Gyr: Early Results from GEMS -- First Phylogenetic Analysis of Galaxy Evolution -- A Unified Picture of Disk Galaxies where Bars, Spirals and Warps Result from the Same Fundamental Causes -- On the Generation of the Hubble Sequence trough an Internal Secular Dynamical Process -- The Angular Momentum Problem and the Formation of Bulgeless Galaxies -- Disks Evolution in a Cosmological Framework --  
505 0 |a X-Ray Perspective of Early Type Galaxies -- Spiral Arm Star Formation in Barred Galaxies -- Galaxy Types and Luminosity Functions in the Soan Digital Sky Survey using Artificial Neural Networks -- Globular Cluster Systems and Supermassive Galactic Black Holes -- Pseudobulges in Barred S0 Galaxies -- Bar and Spiral Torques in the Triangulum Galaxy M33 -- Bar Parameters from Ha Observations Molecular Gas in Classical Elliptical Radio Galaxies -- Bars and Dust Multi Wavelength Maps of Simulations of Galaxy Formation -- How Barred is the NIR Nearby Universe? An Analysis using 2MASS -- Truncation of Stellar Disks at high Redshift Is there a Large Stellar Bar in the LSB Galaxy UGC7321? Spiral structure of the Milky Way: The state of Affairs -- Uncovering Morphology from dust: a NIR View of the Interacting Galaxy Pair NGC5394/95 -- SCUBA Local Universe Galaxy Survey -- How JWST can measure First Light, Reionization and Galaxy Assembly --  
505 0 |a Bulges, Disks and Kinematics of Galaxies at z ~ 1 -- Fourier Decomposition of Galaxies -- The Evolutionary Status of Clusters of Galaxies at z ~ 1 -- Distant z>2 Protoclusters and their Galaxies -- The Galaxy Structure - Redshift Relationship -- The Cosmic Background: Evolution of Infrared Galaxies and Dust Properties -- A lecture Dedicated to the Memory of Mayo Greenberg -- The Physical Evolution of Mass and Dust in Distant Galaxies -- The Warm, Cold and Very Cold Dusty Universe A -- Li Turbulence and Galactic Structure -- Chaos in Spiral Galaxies -- Obtaining Statistics of Turbulent Velocity from Astrophysical Spectral Line Data -- Estimating Power Spectra of Galaxy Structure: Can Statistics Help?- From z>6 to z~2: Unearthing Galaxies at the Edge of the Dark Ages -- Masks in the Milky Way -- The Hierarchical Formation of the Galactic Disk -- The SINGS view of Barred Galaxies -- Quantifying Bar Strength: Morphology Meets Methodology --  
505 0 |a The Warm, Cold and Very Cold Dusty Universe A -- Li Turbulence and Galactic Structure -- Chaos in Spiral Galaxies -- Obtaining Statistics of Turbulent Velocity from Astrophysical Spectral Line Data -- Estimating Power Spectra of Galaxy Structure: Can Statistics Help?- From z>6 to z~2: Unearthing Galaxies at the Edge of the Dark Ages -- Masks in the Milky Way -- The Hierarchical Formation of the Galactic Disk -- The SINGS view of Barred Galaxies -- Quantifying Bar Strength: Morphology Meets Methodology -- Estimation of Bar Strengths from nearby IR Images -- Bar Strengths Measured for the OSUBGS sample: active vs non-active galaxies -- Globular Clusters: Galactic and Internal Motions -- Evolution of Self-Gravitating Gas Disks Driven by a Rotating Bar Potential -- Stellar Disk Truncations: Where do we stand?- On the unification of Dwarf and Giant Elliptical Galaxies -- Photodissociation and the morphology of HI in Galaxies -- The True H2 Content of Spiral Galaxies --  
505 0 |a How Barred is the NIR Nearby Universe? An Analysis using 2MASS -- Truncation of Stellar Disks at high Redshift Is there a Large Stellar Bar in the LSB Galaxy UGC7321? Spiral structure of the Milky Way: The state of Affairs -- Un 
505 0 |a Estimation of Bar Strengths from nearby IR Images -- Bar Strengths Measured for the OSUBGS sample: active vs non-active galaxies -- Globular Clusters: Galactic and Internal Motions -- Evolution of Self-Gravitating Gas Disks Driven by a Rotating Bar Potential -- Stellar Disk Truncations: Where do we stand?- On the unification of Dwarf and Giant Elliptical Galaxies -- Photodissociation and the morphology of HI in Galaxies -- The True H2 Content of Spiral Galaxies -- X-Ray Perspective of Early Type Galaxies -- Spiral Arm Star Formation in Barred Galaxies -- Galaxy Types and Luminosity Functions in the Soan Digital Sky Survey using Artificial Neural Networks -- Globular Cluster Systems and Supermassive Galactic Black Holes -- Pseudobulges in Barred S0 Galaxies -- Bar and Spiral Torques in the Triangulum Galaxy M33 -- Bar Parameters from Ha Observations Molecular Gas in Classical Elliptical Radio Galaxies -- Bars and Dust Multi Wavelength Maps of Simulations of Galaxy Formation --  
505 0 |a Evolution and Impact of Bars over the last nine Gyr: Early Results from GEMS -- First Phylogenetic Analysis of Galaxy Evolution -- A Unified Picture of Disk Galaxies where Bars, Spirals and Warps Result from the Same Fundamental Causes -- On the Generation of the Hubble Sequence trough an Internal Secular Dynamical Process -- The Angular Momentum Problem and the Formation of Bulgeless Galaxies -- Disks Evolution in a Cosmological Framework -- Galaxy Formation and the Cosmological Angular Momentum Problem -- The Problems with Galaxy Formation -- The Interplay between Bars and Dark Matter Halos -- Resent Results from the Spitzer Space Telescope: A New View of Galaxy Morphology and Classification -- Using Bars as Signposts of Galaxy Evolution at High and Low Redshifts -- The VIMOS VLT Deep Survey: Redshift Distribution of a IAB > 24 Sample, and the Effect of Environment on Galaxy Evolution -- An HST AOS/WFC Ha Imaging Survey of Nearby Galaxies -- HST Mid-UV Imaging of Nearby Galaxies --  
505 0 |a Galaxy Formation and the Cosmological Angular MomentumProblem -- The Problems with Galaxy Formation -- The Interplay between Bars and Dark Matter Halos -- Resent Results from the Spitzer Space Telescope: A New View of Galaxy Morphology and Classification -- Using Bars as Signposts of Galaxy Evolution at High and Low Redshifts -- The VIMOS VLT Deep Survey: Redshift Distribution of a IAB > 24 Sample, and the Effect of Environment on Galaxy Evolution -- An HST AOS/WFC Ha Imaging Survey of Nearby Galaxies -- HST Mid-UV Imaging of Nearby Galaxies -- Bulges, Disks and Kinematics of Galaxies at z ~ 1 -- Fourier Decomposition of Galaxies -- The Evolutionary Status of Clusters of Galaxies at z ~ 1 -- Distant z>2 Protoclusters and their Galaxies -- The Galaxy Structure - Redshift Relationship -- The Cosmic Background: Evolution of Infrared Galaxies and Dust Properties -- A lecture Dedicated to the Memory of Mayo Greenberg -- The Physical Evolution of Mass and Dust in Distant Galaxies --  
653 |a Nuclear physics 
653 |a Gravitation 
653 |a Nuclear and Particle Physics 
653 |a Space Physics 
653 |a Classical and Quantum Gravity 
653 |a Astronomy, Cosmology and Space Sciences 
653 |a Astronomy 
653 |a Solar system 
700 1 |a Puerari, Ivânio  |e [editor] 
700 1 |a Freeman, K. C.  |e [editor] 
700 1 |a Groess, R.  |e [editor] 
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520 |a THE EDITORS: DAVID L. BLOCK AND KENNETH C. FREEMAN (SOC CO-CHAIRS), IVANIO PUERARI, ROBERT GROESS AND LIZ K. BLOCK 1. Harvard College Observatory, 1958 The past century has truly brought about an explosive period of growth and discovery for the physical sciences as a whole, and for astronomy in particular. Galaxy morphology has reached a renaissance . . The year: 1958. The date: October 1. The venue: Harvard College Observatory. The lecturer: Walter Baade. With amazing foresight, Baade penned these words: "Young stars, supergiants and so on, make a terrific splash - lots of light. The total mass of these can be very small compared to the total mass of the system". Dr Layzer then asked the key question: " . . . the discussion raises the point of what this classification would look like if you were to ignore completely all the Population I, and just focus attention on the Population II . . . " We stand on the shoulders of giants. The great observer E. E. Barnard, in his pioneering efforts to photograph the Milky Way, devoted the major part of his life to identifying and numbering dusty "holes" and dust lanes in our Milky Way. No one could have dreamt that the pervasiveness of these cosmic dust masks (not only in our Galaxy but also in galaxies at high redshift) is so great, that their "penetration" is truly one of the pioneering challenges from both space-borne telescopes and from the ground