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Showing 1 to 20 of 96 for “"Extragalactic"”.

  1. Extragalactic Globular Cluster Systems

    Das Ziel dieser Dissertation ist die spektroskopische Studie von extragalaktischen Kugelsternhaufensystemen. Ihre Motivation ist das bessere Verstaendnis der Bildung und Entwicklung dieser Kugelsternhaufensysteme und ihrer Wirtsgalaxien. Zu diesem Zweck werden spektroskopische Linienindices des …

    lmu-germany Repository record for Extragalactic Globular Cluster Systems (opens in a new tab)

  2. Extragalactic Novae and Their Progenitors

    … curves far deeper than is typically possible for extragalactic systems.A statistical study was then carried out to test the results of the survey and derive an estimate of the proportion of M31 novae associated with a resolved source in the HST data. This includes, for example, models of the …

    liverpool-jm Repository record for Extragalactic Novae and Their Progenitors (opens in a new tab)

  3. Asymmetries in extragalactic radio sources

    … the three dimensional hydrodynamics of extragalactic radio jets. This entailed putting together a large number of numerical tools before such simulations could be performed. The thesis was structured to be a set of papers, each addressing a computational or astrophysical issue that was …

    uiuc Repository record for Asymmetries in extragalactic radio sources (opens in a new tab)

  4. Starbursts in extragalactic giant H II regions

    Extragalactic giant H II regions (EGHRs) are sites of active, concentrated star formation on manageable scales, and thus provide ideal labs to analyze starburst phenomena. To get a complete picture of the starburst phenomenon, the critical characteristics we must investigate include star formation …

    uiuc Repository record for Starbursts in extragalactic giant H II regions (opens in a new tab)

  5. Extragalactic Radio Sources in Uniform Model Universes

    Made available in DSpace on 2014-12-09T18:34:01Z (GMT). No. of bitstreams: 1 7013456.pdf: 2165188 bytes, checksum: 103532548393fa302ab35585d35fc7e3 (MD5) Previous issue date: 1969

    uiuc Repository record for Extragalactic Radio Sources in Uniform Model Universes (opens in a new tab)

  6. The Luminosity Function of Extragalactic Radio Sources

    Made available in DSpace on 2014-12-05T20:51:49Z (GMT). No. of bitstreams: 1 6305138.pdf: 4472075 bytes, checksum: 7d669eae6b8c4bd5d7775f4188d48ae0 (MD5) Previous issue date: 1963

    uiuc Repository record for The Luminosity Function of Extragalactic Radio Sources (opens in a new tab)

  7. Giant Pair Halos Surrounding Non-Thermal Extragalactic Objects

    Hochenergetische (E>100 GeV) Gammastrahlen aus extragalaktischen Quellen werden infolge der gamma-gamma-Paarbildung (PP) von der kosmischen Infrarot-Hintergrund-strahlung (CIB) absorbiert und loesen elektromagnetische Schauer durch Paarbildung und inverse Comptonstreuung aus. Dies fuehrt zur …

    heid-diss Repository record for Giant Pair Halos Surrounding Non-Thermal Extragalactic Objects (opens in a new tab)

  8. Structural and Photometric Properties of Extragalactic Stellar Spheroids

    After an overview of the science of galaxy morphology, a new classification for galactic form, based upon the Yerkes system, is presented. This classification scheme is then applied to the study of the role of environment in determining the nature of galaxy populations. By examining the …

    uiuc Repository record for Structural and Photometric Properties of Extragalactic Stellar Spheroids (opens in a new tab)

  9. The Universality of Intrinsic Flattening in Extragalactic Stellar Disks

    Highly inclined (edge-on) galaxies provide the unique perspective necessary to constrain the intrinsic flattening, 𝑐/𝑎, of galactic disks. We use “dust-free” 3.6 𝜇m maps of 141 edge-on spiral galaxies from the Spitzer Survey of Stellar Structure in Galaxies (S4G) and its early-type galaxy extension …

    queens Repository record for The Universality of Intrinsic Flattening in Extragalactic Stellar Disks (opens in a new tab)

  10. Improving the extragalactic distance scale using Cepheids in M33

    … as Cepheids are used to tie down the base of the extragalactic distance scale. Without an accurate calibration for the nearest distances, the distances we measure for all other objects will be subject to systematic uncertainties. This thesis studies how the chemical composition of a Cepheid …

    liverpool-jm Repository record for Improving the extragalactic distance scale using Cepheids in M33 (opens in a new tab)

  11. The formation and evolution of massive clusters in extragalactic environments

    There are a host of open questions in the study of massive clusters relating to cluster formation and evolution. Understanding these processes can be useful in studying their host galaxies and how they have evolved. The formation of globular clusters is also a well debated topic, which is yet …

    liverpool-jm Repository record for The formation and evolution of massive clusters in extragalactic environments (opens in a new tab)

  12. Detecting and understanding extragalactic Lyman α emission using 3D spectroscopy

    In this thesis we use integral-field spectroscopy to detect and understand of Lyman α (Lyα) emission from high-redshift galaxies. Intrinsically the Lyα emission at λ = 1216 Å is the strongest recombination line from galaxies. It arises from the 2p → 1s transition in hydrogen. In star-forming …

    potsdam-diss Repository record for Detecting and understanding extragalactic Lyman α emission using 3D spectroscopy (opens in a new tab)

  13. Spectral characteristics of low-frequency variability in compact extragalactic radio sources

    … of the observed fluctuations. Plane waves from extragalactic radio sources propagating through the interstellar medium, a medium with fluctuations of the refractive index due to electron density irregularities, emerge from that medium corrugated. Since fluctuations present on scales greater than …

    vt Repository record for Spectral characteristics of low-frequency variability in compact extragalactic radio sources (opens in a new tab)

  14. Multi-Wavelength Extragalactic Surveys: Star Formation of IR-Submm Selected Galaxies

    This Thesis aims to identify and analyse galaxy populations over a range of redshifts in order to evaluate the star formation history over cosmic time. Explicitly focusing on the infrared to submillimetre regime, I carried out a comprehensive multi-wavelength approach at the North and South …

    the-open-u Repository record for Multi-Wavelength Extragalactic Surveys: Star Formation of IR-Submm Selected Galaxies (opens in a new tab)

  15. Wideband spectropolarimetry of extragalactic radio sources with KAT 7 and commissioning phase MeerKAT

    The study of cosmic magnetism is vital in fully understanding the role that magnetic fields play in the evolution of cosmological objects such as galaxies. The exact role played by magnetism in galaxy evolution is still not fully understood. This work aims to use wide band radio polarimetry to …

    cape-town Repository record for Wideband spectropolarimetry of extragalactic radio sources with KAT 7 and commissioning phase MeerKAT (opens in a new tab)

  16. The nature and evolution of I. extragalactic radio sources, and II. young stellar clusters

    Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1998.

    mit Repository record for The nature and evolution of I. extragalactic radio sources, and II. young stellar clusters (opens in a new tab)

  17. Test of the Infrared Wide-Field Camera OMEGA2000 and its Application for an Extragalactic Survey

    OMEGA2000 is a prime-focus, near-infrared, wide-field camera, mounted on the 3. 5m telescope at Calar Alto. The camera uses a 2kx2k HAWAII-2 Focal plane array with a sensitivity from z to K band. In the first part of the thesis, we discuss the work aimed at optimizing the operation of the HAWAII-2 …

    heid-diss Repository record for Test of the Infrared Wide-Field Camera OMEGA2000 and its Application for an Extragalactic Survey (opens in a new tab)

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