The IGM/galaxy connection : the distribution of baryons at z=0

By J. Rosenberg, M. Putman. 2003

165 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/b544784cbd7bf596cc6ce5179c0e445cbb4a7010

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Citations in the corpus

• Moving mesh cosmology: tracing cosmological gas accretion (2013, background): “Numerical simulations over the past decade have shown evidence for a cold accretion mode which dominates both at high redshift and for low mass objects at late times (Katz et al. 2003; Kereš et al. 2005, 2009; Ocvirk et al. 2008).”
• The physics of the intergalactic medium (2007, background): “Reviews of the low redshift IGM are provided by Shull (2003) and Stocke et al. (2006b).”
• THE RELATION BETWEEN STAR FORMATION RATE AND STELLAR MASS FOR GALAXIES AT 3.5 ⩽ z ⩽ 6.5 IN CANDELS (2014, unknown): “…are subdominant to galaxy growth at high redshift z > 2 (Murali et al. 2002; Kereš et al. 2005) and the SFR tracks the gas accretion rate (Birnboim & Dekel 2003; Katz et al. 2003; Kereš et al. 2005; Dekel et al. 2009; Bouché et al. 2010; Ceverino et al. 2010; FaucherGiguère et al. 2011).”
• The Search for the Missing Baryons at Low Redshift (2007, background): “Both groups agree that the OVII Kα (21.60 Å) and the OVIII Kα (18.97 Å) lines are detected in PKS 2155-304, although Nicastro et al. (2002) report the detection of a Ne IX Kα (13.45 Å) while Rasmussen et al. (2003) report an upper limit.”
• Mass, metal, and energy feedback in cosmological simulations (2007, background): “0.5, leading to a value consistent within the error bars of z ≈ 0 measurement by Frye et al. (2003).”
• A High Spatial Resolution X-Ray and Hα Study of Hot Gas in the Halos of Star-forming Disk Galaxies. II. Quantifying Supernova Feedback (2003, background): “Depending on the exact model assumed, the mass of gas in the halo of a Milky Way–like galaxy prior to any starburst ranges from a few times 107 to a few times 108M (see models 4 and 5 in Strickland et al. 2002).”
• THE COSMOS2015 CATALOG: EXPLORING THE 1 < z < 6 UNIVERSE WITH HALF A MILLION GALAXIES (2016, background): “However, recent hydrodynamical simulations now suggest however now that most of the gas is accreted directly from cold dense filaments without being shockheated (Katz et al. 2003; Kereš et al. 2005; Ocvirk et al. 2008; Dekel et al. 2009) at least for lower-mass haloes at high redshift.”
• The Low-z Intergalactic Medium. III. H I and Metal Absorbers at z < 0.4 (2007, methodology): “However, most of these baryons do not exist in collapsed form, and probably are distributed throughout various phases of the IGM (Cen & Ostriker 1999; Shull 2003).”
• The Secular Evolution of Disk Structural Parameters (2005, background): “…the smooth accretion of gas cooling inside the dark halo (combined with the accretion along cold filaments for lower mass objects; Katz & Gunn 1991; Katz et al. 2003; Birnboim & Dekel 2003; Kereš et al. 2005) following an intense phase of merger activity that can give rise to the stellar halo and…”