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Showing 1 to 20 of 131 for “"metallicity"”.

  1. Metallicity correlations in galaxies

    … tool for extracting information from the 2D metallicity maps that integral field spectroscopy produces. Using the current integrated field unit observations and simulations, this thesis tries to gradually investigate the following aspects. I show that two-point correlations of current …

    aus-cath Repository record for Metallicity correlations in galaxies (opens in a new tab)

  2. Metallicity correlations in galaxies

    … tool for extracting information from the 2D metallicity maps that integral field spectroscopy produces. Using the current integrated field unit observations and simulations, this thesis tries to gradually investigate the following aspects. I show that two-point correlations of current …

    anu Repository record for Metallicity correlations in galaxies (opens in a new tab)

  3. Massive stars in low metallicity environments

    … sensitive to mass loss, internal mixing, metallicity, rotation, binarity, and magnetic fields. In this thesis, I have probed the evolution of massive stars for a range of metallicities, including our Milky Way galaxy and the Magellanic Clouds. This work provides an insight into the …

    qu-belfast Repository record for Massive stars in low metallicity environments (opens in a new tab)

  4. Shocks and Metallicity Gradients in Normal Star-Forming Galaxies

    … explores gas flows in local galaxies by studying metallicity gradients and galactic- scale outflows in normal star-forming galaxies. This is made possible by new integral field spectroscopy data that provide simultaneously spatial and spectral information of galaxies. First, I measure metallicity

    hawaii Repository record for Shocks and Metallicity Gradients in Normal Star-Forming Galaxies (opens in a new tab)

  5. THE CEPHEIDS OF M33: DISTANCE AND METALLICITY EFFECTS THROUGH SLOAN FILTERS

    … are therefore imparted with varying levels of metallicity. The difference in Cepheid metallicities may give rise to variations in their observable characteristics, leading to changes in the Leavitt Law. These changes may manifest themselves as a metallicity dependence on the slope or zero-point …

    liverpool-jm Repository record for THE CEPHEIDS OF M33: DISTANCE AND METALLICITY EFFECTS THROUGH SLOAN FILTERS (opens in a new tab)

  6. Kinematics and metallicity of RGB stars in the triangulum (M33) galaxy

    cambridge

  7. Probing the history of galaxy clusters with metallicity and entropy measurements

    … spatially resolved measurements of their metallicity and entropy content. A sample of 45 nearby clusters observed with Chandra is analyzed to produce radial density, temperature, entropy and metallicity profiles. The entropy profiles are computed to larger radial extents than in previous …

    mit Repository record for Probing the history of galaxy clusters with metallicity and entropy measurements (opens in a new tab)

  8. The effective temperatures and physical properties of red supergiants : the effects of metallicity.

    … to demonstrate a correlation between galactic metallicity and the average spectral subtype of a galaxy's RSG population. Research contained in this thesis has been published in part by the Astrophysical Journal, v. 628, p. 973 Research contained in this thesis has been submitted to the …

    mit Repository record for The effective temperatures and physical properties of red supergiants : the effects of metallicity. (opens in a new tab)

  9. On the evolution of star forming galaxies : the metallicity of dwarfs and the effect of environment on local luminous IR galaxies

    … "On evolution of star forming galaxies: the metallicity of dwarfs and the effect of environment on local luminous infrared galaxies" is divided into two main areas. First a detailed study of the environment and star formation relationship of local Luminous Infrared Galaxies (LIRGs), with …

    cape-town Repository record for On the evolution of star forming galaxies : the metallicity of dwarfs and the effect of environment on local luminous IR galaxies (opens in a new tab)

  10. The stellar halos of Milky Way type galaxies in the EAGLE simulations

    … of MW-mass disc galaxy stellar halos. Negative metallicity gradients are ubiquitous in the galaxy samples analysed, with gradients in the range -0.002 to -0.02 dex/kpc, consistent with recent observations of M31. The gradient was found to be primarily driven by the transition from high …

    liverpool-jm Repository record for The stellar halos of Milky Way type galaxies in the EAGLE simulations (opens in a new tab)

  11. The structure of the Large Magellanic Cloud

    This work gives an account of the study of the metallicity [Fe/H] distribution (gradient) in the oldest population in the Large Magellanic Cloud (LMC), by making use of the available RR Lyrae data from the Optical Gravitational Lensing Experiment III (OGLE III). RR Lyrae stars are amongst the …

    cape-town Repository record for The structure of the Large Magellanic Cloud (opens in a new tab)

  12. The structure of the large magellanic cloud

    This work gives an account of the study of the metallicity [Fe/H] distribution (gradient) in the oldest population in the Large Magellanic Cloud (LMC), by making use of the available RR Lyrae data from the Optical Gravitational Lensing Experiment III (OGLE III). RR Lyrae stars are amongst the …

    cape-town Repository record for The structure of the large magellanic cloud (opens in a new tab)

  13. The accuracy of integrated star clusters parameters. The effects of stochasticity /

    … physical parameters (age, mass, extinction, and metallicity) of star clusters with integrated broad-band photometry are traditionally derived using the Simple Stellar Population models (SSP). However, parameters are inaccurate because the models do not take the stochastic sampling of star mass in …

    vilnius Repository record for The accuracy of integrated star clusters parameters. The effects of stochasticity / (opens in a new tab)

  14. Integralinių žvaigždžių spiečių parametrų tikslumas. Stochastiniai efektai /

    … physical parameters (age, mass, extinction, and metallicity) of star clusters with integrated broad-band photometry are traditionally derived using the Simple Stellar Population models (SSP). However, parameters are inaccurate because the models do not take the stochastic sampling of star mass in …

    vilnius Repository record for Integralinių žvaigždžių spiečių parametrų tikslumas. Stochastiniai efektai / (opens in a new tab)

  15. Metallicities and stellar populations in spiral bulges

    … stellar populations of approximately solar metallicity or above. In bulges, central line-strengths are shown to lie close to, or within, the loci defining solar abundance ratio SSPs. The large number (24) of indices measured in this study, in conjunction with models of the effects of varying …

    cent-lancashire Repository record for Metallicities and stellar populations in spiral bulges (opens in a new tab)

  16. New Insights on the Evolutionary Mechanisms of Local and Distant Galaxies

    … metallicities and the real drivers of the mass-metallicity relation (MZR) and fundamental metallicity relation (FMR) on both resolved and global scales. I find evidence for a resolved version of the FMR and also that local metallicity depends on both local and global galactic properties, hence …

    cambridge Repository record for New Insights on the Evolutionary Mechanisms of Local and Distant Galaxies (opens in a new tab)

  17. Chemodynamical Adaptive Mesh Refinement Simulations of Disk Galaxies

    … is used to compare properties such as the metallicity gradients and morphology to determine if systematic differences are apparent as a function of subtle environmental differences. Almost no distinction is seen between galaxies in the field and the loose group environments: individual …

    cent-lancashire Repository record for Chemodynamical Adaptive Mesh Refinement Simulations of Disk Galaxies (opens in a new tab)

  18. Improving the extragalactic distance scale using Cepheids in M33

    … arisen in its calibration, namely the effect of metallicity on the period-luminosity relation. It is important that we quantify this effect 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 …

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

  19. Planets around cool stars: a spectroscopic and photometric study of M dwarfs and their planets

    … poorly established stellar parameters (radius, metallicity, etc.). For this dissertation I have worked to mitigate these problems with the goals of finding new transiting planets and establishing the role of stellar metallicity on the size and occurrence of transiting planets around M dwarfs. I …

    hawaii Repository record for Planets around cool stars: a spectroscopic and photometric study of M dwarfs and their planets (opens in a new tab)

  20. Evolution of Galaxies - Star Formation Histories in Nearby Spheroids

    … particularly sensitive to a galaxy's age and metallicity were measured as equivalent widths and then calibrated to the common scale of the Lick Indices. The Lick Indices were used in deriving all key results throughout the thesis. The modelled sample of galaxies from Proctor & Sansom (2002) …

    cent-lancashire Repository record for Evolution of Galaxies - Star Formation Histories in Nearby Spheroids (opens in a new tab)

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