Essays about: "galaxies: high-redshift"
Showing result 1 - 5 of 10 essays containing the words galaxies: high-redshift.
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1. Searching for direct collapse black holes using the James Webb Space Telescope
University essay from Uppsala universitet/Institutionen för fysik och astronomiAbstract : Recent detections of massive quasars at z > 6 has proven to be an interesting challengefor cosmology given the short time frame that these objects have to reach a certainmass via conventional methods (e.g., galaxy mergers). READ MORE
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2. Colliding Galaxies in a (Nut)Shell
University essay from Lunds universitet/Astronomi - Genomgår omorganisation; Lunds universitet/Fysiska institutionenAbstract : Galaxy interactions and mergers are natural recurring events in the current cosmological paradigm, events that often coincide with starbursts and enhanced star formation activity. To understand why that is, one can use idealised (non-cosmological) merger simulations, which provide freedom to recreate specific tidally distorted galaxies, and analysis of the time evolution and underlying physics of the star formation activity at a high spatial resolution. READ MORE
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3. High Redshift Galaxies with JWST and Euclid
University essay from Uppsala universitet/Institutionen för fysik och astronomiAbstract : This projects studies which early galaxy populations will be visible using the telescopes JWST and Euclid. Galaxy luminosity functions are calculated for different redshifts, with the galaxy number density as a function of apparent magnitude. The apparent magnitude is used to enable easy comparisons with the observational limits of JWST and Euclid. READ MORE
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4. Measuring the [C II]-to-H I connection in high-redshift absorption-selected galaxies
University essay from Lunds universitet/Astronomi - Genomgår omorganisationAbstract : HI neutral gas is the basic building block of galaxies. It dictates the star formation rate and hence the metal enrichment rates within high redshift galaxies. HI neutral gas cannot be directly observed beyond z ≈ 0. READ MORE
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5. Study of CO Emission in Nine Hot Dust-Obscured Galaxies at z ∼3
University essay from Uppsala universitet/Institutionen för fysik och astronomiAbstract : Massive galaxies evolve through different phases including starburst-dominated and active galactic nuclei (AGN)-dominated phases. These phases are predicted to be prevalent at earlier times (z ∼ 2 − 3). READ MORE