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  • 1
    Online Resource
    Online Resource
    Outskirts of Galaxies / (2017)
    Cham :Springer,
    Details
    UID:
    almafu_BV044432742
    Format: 1 Online-Ressource (XI, 362 p. 94 illus., 65 illus. in color).
    ISBN: 978-3-319-56570-5
    Series Statement: Astrophysics and Space Science Library volume 434
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 978-3-319-56569-9
    Language: English
    DOI: 10.1007/978-3-319-56570-5
    URL: Volltext  (URL des Erstveröffentlichers)
    URL: lizenzpflichtig
    URL: Volltext  (lizenzpflichtig)
    URL: Cover
    Library Location Call Number Volume/Issue/Year Availability
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    Online Access
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    FU Berlin
    UB Potsdam
    Charité
  • 2
    Online Resource
    Online Resource
    Secular evolution in galaxies : properties of bars and bulges as seen with integral field spectroscopy (2019)
    Potsdam
    Details
    UID:
    gbv_1745276297
    Format: 1 Online-Ressource (viii, 97 Seiten, 15688 KB) , Illustrationen, Diagramme
    Content: Galaxies are gravitationally bound systems of stars, gas, dust and - probably - dark matter. They are the building blocks of the Universe. The morphology of galaxies is diverse: some galaxies have structures such as spirals, bulges, bars, rings, lenses or inner disks, among others. The main processes that characterise galaxy evolution can be separated into fast violent events that dominated evolution at earlier times and slower processes, which constitute a phase called secular evolution, that became dominant at later times. Internal processes of secular evolution include the gradual rearrangement of matter and angular momentum, the build-up and dissolution of substructures or the feeding of supermassive black holes and their feedback. Galaxy bulges – bright central components in disc galaxies –, on one hand, are relics of galaxy formation and evolution. For instance, the presence of a classical bulge suggests a relatively violent history. In contrast, the presence of a disc-like bulge instead indicates the occurrence of secular ...
    Note: Dissertation Universität Potsdam 2020
    Additional Edition: Erscheint auch als Druck-Ausgabe Neumann, Justus Secular evolution in galaxies Potsdam, 2019
    Language: English
    Keywords: Hochschulschrift
    DOI: 10.25932/publishup-48270
    URN: urn:nbn:de:kobv:517-opus4-482701
    URL: kostenfrei
    URL: kostenfrei
    Author information: Wisotzki, Lutz
    Author information: Steinmetz, Matthias 1966-
    Library Location Call Number Volume/Issue/Year Availability
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    Open Access Request
    UB Potsdam
  • 3
    Book
    Book
    Secular evolution in galaxies : properties of bars and bulges as seen with integral field spectroscopy (2019)
    Potsdam
    Details
    UID:
    gbv_1745283013
    Format: viii, 97 Seiten , Illustrationen, Diagramme
    Content: Galaxies are gravitationally bound systems of stars, gas, dust and - probably - dark matter. They are the building blocks of the Universe. The morphology of galaxies is diverse: some galaxies have structures such as spirals, bulges, bars, rings, lenses or inner disks, among others. The main processes that characterise galaxy evolution can be separated into fast violent events that dominated evolution at earlier times and slower processes, which constitute a phase called secular evolution, that became dominant at later times. Internal processes of secular evolution include the gradual rearrangement of matter and angular momentum, the build-up and dissolution of substructures or the feeding of supermassive black holes and their feedback. Galaxy bulges – bright central components in disc galaxies –, on one hand, are relics of galaxy formation and evolution. For instance, the presence of a classical bulge suggests a relatively violent history. In contrast, the presence of a disc-like bulge instead indicates the occurrence of secular ...
    Note: Dissertation Universität Potsdam 2020
    Additional Edition: Erscheint auch als Online-Ausgabe Neumann, Justus Secular evolution in galaxies Potsdam, 2019
    Language: English
    Keywords: Hochschulschrift
    URL: Inhaltsverzeichnis
    Author information: Wisotzki, Lutz
    Author information: Steinmetz, Matthias 1966-
    Library Location Call Number Volume/Issue/Year Availability
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    Book
    UB Potsdam get availability status
  • 4
    Online Resource
    Online Resource
    Secular evolution of galaxies / (2012)
    Cambridge ; : Cambridge University Press,
    Details
    UID:
    almahu_9948317963102882
    Format: 1 online resource (658 pages) : , illustrations (some color).
    ISBN: 9781107248779 (e-book)
    Series Statement: Canary Islands Winter School of Astrophysics ; Volume XXIII
    Note: Secular evolution in disk galaxies / John Kormendy -- Galaxy morphology / Ronald J. Buta -- Dynamics of secular evolution / James Binney -- Bars and secular evolution in disk galaxies : theoretical input / E. Athanassoula -- Stellar populations / Reynier F. Peletier -- Star formation rate indicators / Daniela Calzetti -- The evolving interstellar medium / Jacqueline van Gorkom -- Evolution of star formation and gas / Nick Z. Scoville -- Cosmological evolution of galaxies / Isaac Shlosman.
    Additional Edition: Print version: Secular evolution of galaxies. Cambridge : Cambridge University Press, 2012 ISBN 9781107035270
    Language: English
    Keywords: Electronic books.
    URL: Click to View
    Library Location Call Number Volume/Issue/Year Availability
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    Online Resource
    HU Berlin
  • 5
    Online Resource
    Online Resource
    Outskirts of Galaxies / (2017)
    Cham :Springer,
    Details
    UID:
    edoccha_BV044432742
    Format: 1 Online-Ressource (XI, 362 p. 94 illus., 65 illus. in color).
    ISBN: 978-3-319-56570-5
    Series Statement: Astrophysics and Space Science Library volume 434
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 978-3-319-56569-9
    Language: English
    DOI: 10.1007/978-3-319-56570-5
    URL: Volltext  (URL des Erstveröffentlichers)
    Library Location Call Number Volume/Issue/Year Availability
    BibTip Others were also interested in ...
    Online Resource
    Online Access
    Open Access Request
    Charité
  • 6
    Online Resource
    Online Resource
    Outskirts of Galaxies / (2017)
    Cham :Springer,
    Details
    UID:
    edocfu_BV044432742
    Format: 1 Online-Ressource (XI, 362 p. 94 illus., 65 illus. in color).
    ISBN: 978-3-319-56570-5
    Series Statement: Astrophysics and Space Science Library volume 434
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 978-3-319-56569-9
    Language: English
    DOI: 10.1007/978-3-319-56570-5
    URL: Volltext  (URL des Erstveröffentlichers)
    Library Location Call Number Volume/Issue/Year Availability
    BibTip Others were also interested in ...
    Online Resource
    Online Access
    Open Access Request
    FU Berlin
  • 7
    Online Resource
    Online Resource
    Secular evolution of galaxies (2012)
    Cambridge : Cambridge University Press
    Details
    UID:
    gbv_883347857
    Format: 1 Online-Ressource (xvii, 638 pages) , digital, PDF file(s)
    ISBN: 9781139547420
    Series Statement: Canary Islands Winter School of Astrophysics
    Content: The formation and evolution of galaxies is one of the most important topics in astrophysics. Secular evolution refers to the relatively slow dynamical evolution due to internal processes induced by a galaxy's spiral arms, bars, galactic winds, black holes and dark matter haloes. It plays an important role in the evolution of spiral galaxies with major consequences for galactic bulges, the transfer of angular momentum, and the distribution of a galaxy's constituent stars, gas and dust. This internal evolution is key to understanding cosmological models of galaxy formation and evolution. Based on the twenty-third Winter School of the Canary Islands Institute of Astrophysics, this volume presents reviews from nine experts on the observational and theoretical research into secular processes, and what these processes can tell us about the structure and formation of galaxies. The volume provides a grounding for graduate students and researchers working on galactic dynamics and galaxy evolution
    Content: Secular evolution in disk galaxies / John Kormendy -- Galaxy morphology / Ronald J. Buta -- Dynamics of secular evolution / James Binney -- Bars and secular evolution in disk galaxies : theoretical input / E. Athanassoula -- Stellar populations / Reynier F. Peletier -- Star formation rate indicators / Daniela Calzetti -- The evolving interstellar medium / Jacqueline van Gorkom -- Evolution of star formation and gas / Nick Z. Scoville -- Cosmological evolution of galaxies / Isaac Shlosman
    Note: Title from publisher's bibliographic system (viewed on 05 Oct 2015)
    Additional Edition: ISBN 9781107035270
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 9781107035270
    Language: English
    DOI: 10.1017/CBO9781139547420
    URL: Volltext
    Library Location Call Number Volume/Issue/Year Availability
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    Online Resource
    Online Access
    Open Access Request
    UB Potsdam
  • 8
    Online Resource
    Online Resource
    Secular evolution of galaxies / (2012)
    Cambridge :Cambridge University Press,
    Details
    UID:
    almafu_9959237442202883
    Format: 1 online resource (xvii, 638 pages) : , digital, PDF file(s).
    Edition: 1st ed.
    ISBN: 1-139-89160-X , 1-107-25126-5 , 1-107-24877-9 , 1-107-25043-9 , 1-139-54742-9 , 1-107-24794-2 , 1-107-24960-0
    Series Statement: Canary Islands Winter School of Astrophysics
    Content: The formation and evolution of galaxies is one of the most important topics in astrophysics. Secular evolution refers to the relatively slow dynamical evolution due to internal processes induced by a galaxy's spiral arms, bars, galactic winds, black holes and dark matter haloes. It plays an important role in the evolution of spiral galaxies with major consequences for galactic bulges, the transfer of angular momentum, and the distribution of a galaxy's constituent stars, gas and dust. This internal evolution is key to understanding cosmological models of galaxy formation and evolution. Based on the twenty-third Winter School of the Canary Islands Institute of Astrophysics, this volume presents reviews from nine experts on the observational and theoretical research into secular processes, and what these processes can tell us about the structure and formation of galaxies. The volume provides a grounding for graduate students and researchers working on galactic dynamics and galaxy evolution.
    Note: Title from publisher's bibliographic system (viewed on 05 Oct 2015). , Secular evolution in disk galaxies / John Kormendy -- Galaxy morphology / Ronald J. Buta -- Dynamics of secular evolution / James Binney -- Bars and secular evolution in disk galaxies : theoretical input / E. Athanassoula -- Stellar populations / Reynier F. Peletier -- Star formation rate indicators / Daniela Calzetti -- The evolving interstellar medium / Jacqueline van Gorkom -- Evolution of star formation and gas / Nick Z. Scoville -- Cosmological evolution of galaxies / Isaac Shlosman. , English
    Additional Edition: ISBN 1-107-03527-9
    Additional Edition: ISBN 1-306-07169-0
    Language: English
    Library Location Call Number Volume/Issue/Year Availability
    BibTip Others were also interested in ...
    Online Resource
    FU Berlin
  • 9
    Online Resource
    Online Resource
    Secular evolution of galaxies / (2012)
    Cambridge :Cambridge University Press,
    Details
    UID:
    almahu_9948233649402882
    Format: 1 online resource (xvii, 638 pages) : , digital, PDF file(s).
    ISBN: 9781139547420 (ebook)
    Series Statement: Canary Islands Winter School of Astrophysics
    Content: The formation and evolution of galaxies is one of the most important topics in astrophysics. Secular evolution refers to the relatively slow dynamical evolution due to internal processes induced by a galaxy's spiral arms, bars, galactic winds, black holes and dark matter haloes. It plays an important role in the evolution of spiral galaxies with major consequences for galactic bulges, the transfer of angular momentum, and the distribution of a galaxy's constituent stars, gas and dust. This internal evolution is key to understanding cosmological models of galaxy formation and evolution. Based on the twenty-third Winter School of the Canary Islands Institute of Astrophysics, this volume presents reviews from nine experts on the observational and theoretical research into secular processes, and what these processes can tell us about the structure and formation of galaxies. The volume provides a grounding for graduate students and researchers working on galactic dynamics and galaxy evolution.
    Note: Title from publisher's bibliographic system (viewed on 05 Oct 2015). , Secular evolution in disk galaxies / John Kormendy -- Galaxy morphology / Ronald J. Buta -- Dynamics of secular evolution / James Binney -- Bars and secular evolution in disk galaxies : theoretical input / E. Athanassoula -- Stellar populations / Reynier F. Peletier -- Star formation rate indicators / Daniela Calzetti -- The evolving interstellar medium / Jacqueline van Gorkom -- Evolution of star formation and gas / Nick Z. Scoville -- Cosmological evolution of galaxies / Isaac Shlosman.
    Additional Edition: Print version: ISBN 9781107035270
    Language: English
    URL: https://doi.org/10.1017/CBO9781139547420
    Library Location Call Number Volume/Issue/Year Availability
    BibTip Others were also interested in ...
    Online Resource
    HU Berlin
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