The First Galaxies

By J. Dunlop. 2012

402 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/6255b0f137b0ee6bc961fa4303cb81ef57e45267

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. R. Bouwens
2. P. Hopkins
3. Richard S. Ellis
4. D. Stark
5. J. Dunlop
6. P. Oesch
7. R. McLure
8. Brant Robertson

Citations in the corpus

• Primordial star formation under the influence of far ultraviolet radiation: 1540 cosmological haloes and the stellar mass distribution (2015, background): “Primordial stars play vital roles in the early evolution of the cosmos by initiating cosmic reionization and chemical enrichment of the inter-galactic medium (e.g., Bromm & Yoshida 2011).”
• CONTRASTING GALAXY FORMATION FROM QUANTUM WAVE DARK MATTER, ψDM, WITH ΛCDM, USING PLANCK AND HUBBLE DATA (2015, background): “…remains very challenging when incorporating all relevant processes which may affect ultraviolet (UV) ionization (e.g., Springel & Hernquist 2003; Bromm & Yoshida 2011; Wise et al. 2014), including early galactic outflows (e.g., Frye et al. 2002) and their feedback effects (e.g., Scannapieco &…”
• Possible indirect confirmation of the existence of Pop III massive stars by gravitational wave (2014, background): “Moreover, cosmological simulations studying the hierarchically merging of haloes suggest that most galaxies could include a large number of the mini-haloes where Pop III stars form (e.g. Greif et al. 2008; Bromm & Yoshida 2011; Rashkov et al. 2012).”
• DWARF GALAXIES WITH OPTICAL SIGNATURES OF ACTIVE MASSIVE BLACK HOLES (2013, background): “…in present-day dwarf galaxies, we will gain insight into whether seed BHs formed primarily as the end-product of Population III stars (e.g., Bromm & Yoshida 2011), in a direct collapse scenario (e.g., Haehnelt & Rees 1993; Lodato & Natarajan 2006; Begelman et al. 2006), or in a runaway…”
• The First Billion Years project: the impact of stellar radiation on the co-evolution of Populations II and III (2012, background): “This sets the stage for the onset of metal-enriched, Pop II star formation (e.g. Wise & Abel 2008; Greif et al. 2010; Maio et al. 2011) in the first galaxies (e.g. Bromm & Yoshida 2011).”
• The birth of a galaxy – II. The role of radiation pressure (2012, background): “1010 (Bromm & Yoshida 2011) are an excellent cosmological testbed to numerically investigate the impact of each physical process.”
• Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies (2013, background): “The formation of the first stars has been studied in theoretical detail (e.g., Ferrara 1998; Abel, Bryan & Norman 2000; Bromm & Yoshida 2011), but their typical masses [or initial mass function (IMF)] have not been clarified yet.”
• WHAT NEXT-GENERATION 21 cm POWER SPECTRUM MEASUREMENTS CAN TEACH US ABOUT THE EPOCH OF REIONIZATION (2013, background): “Observationally, the redshift of EoR is roughly constrained to be between z ∼ 6–13, with a likely extended duration; see Furlanetto et al. (2006b), Barkana & Loeb (2007), and Loeb & Furlanetto (2013) for reviews of the field.”
• Blossoms from black hole seeds: properties and early growth regulated by supernova feedback (2016, background): “Observational evidence on the initial mass function (IMF) of PopIII stars are lacking, but theoretical studies suggest that they could have masses in the range 10 − 1000 M (Bromm & Yoshida 2011; Hirano et al. 2014).”
• CLASH: THREE STRONGLY LENSED IMAGES OF A CANDIDATE z ≈ 11 GALAXY (2012, background): “470 million years old (Wise & Abel 2007; Wise et al. 2008; Greif et al. 2008, 2010; and for recent reviews, see Bromm & Yoshida 2011 and Dunlop 2012).”
• THE ABUNDANCE OF STAR-FORMING GALAXIES IN THE REDSHIFT RANGE 8.5–12: NEW RESULTS FROM THE 2012 HUBBLE ULTRA DEEP FIELD CAMPAIGN (2012, background): “During this time, star-forming galaxies likely played a significant role in completing the reionization of intergalactic hydrogen (Robertson et al. 2010a; Bromm & Yoshida 2011; Dunlop 2012).”
• Gravitational probes of dark matter physics (2017, background): “Galaxies form from gas enriched by the first generation of stars, and cannot form in arbitrarily small halos [389, 390].”