FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2418080963> ?p ?o ?g. }

• W2418080963 endingPage "1521" @default.
• W2418080963 startingPage "1505" @default.
• W2418080963 abstract "We present full volume cosmological simulations using the moving-mesh code AREPO to study the coevolution of dust and galaxies. We extend the dust model in AREPO to include thermal sputtering of grains and investigate the evolution of the dust mass function, the cosmic distribution of dust beyond the interstellar medium, and the dependence of dust-to-stellar mass ratio on galactic properties. The simulated dust mass function is well-described by a Schechter fit and lies closest to observations at $z = 0$. The radial scaling of projected dust surface density out to distances of $10 , text{Mpc}$ around galaxies with magnitudes $17 < i < 21$ is similar to that seen in Sloan Digital Sky Survey data, albeit with a lower normalisation. At $z = 0$, the predicted dust density of $Omega_text{dust} approx 1.3 times 10^{-6}$ lies in the range of $Omega_text{dust}$ values seen in low-redshift observations. We find that dust-to-stellar mass ratio anti-correlates with stellar mass for galaxies living along the star formation main sequence. Moreover, we estimate the $850 , mutext{m}$ number density functions for simulated galaxies and analyse the relation between dust-to-stellar flux and mass ratios at $z = 0$. At high redshift, our model fails to produce enough dust-rich galaxies, and this tension is not alleviated by adopting a top-heavy initial mass function. We do not capture a decline in $Omega_text{dust}$ from $z = 2$ to $z = 0$, which suggests that dust production mechanisms more strongly dependent on star formation may help to produce the observed number of dusty galaxies near the peak of cosmic star formation." @default.
• W2418080963 created "2016-06-24" @default.
• W2418080963 creator A5005759342 @default.
• W2418080963 creator A5039703536 @default.
• W2418080963 creator A5066497572 @default.
• W2418080963 creator A5085246344 @default.
• W2418080963 creator A5087694114 @default.
• W2418080963 date "2017-02-23" @default.
• W2418080963 modified "2023-10-13" @default.
• W2418080963 title "Simulating the dust content of galaxies: successes and failures" @default.
• W2418080963 cites W1484400061 @default.
• W2418080963 cites W1494146418 @default.
• W2418080963 cites W1681063222 @default.
• W2418080963 cites W1799178968 @default.
• W2418080963 cites W1859386239 @default.
• W2418080963 cites W1869477344 @default.
• W2418080963 cites W1911876284 @default.
• W2418080963 cites W1918040529 @default.
• W2418080963 cites W1925665838 @default.
• W2418080963 cites W1941318275 @default.
• W2418080963 cites W1943043803 @default.
• W2418080963 cites W1952356865 @default.
• W2418080963 cites W1964679725 @default.
• W2418080963 cites W1966856883 @default.
• W2418080963 cites W1967137433 @default.
• W2418080963 cites W1969141849 @default.
• W2418080963 cites W1973808059 @default.
• W2418080963 cites W1974288578 @default.
• W2418080963 cites W1975549749 @default.
• W2418080963 cites W1975983552 @default.
• W2418080963 cites W1977843574 @default.
• W2418080963 cites W1980927133 @default.
• W2418080963 cites W1983217322 @default.
• W2418080963 cites W1985720489 @default.
• W2418080963 cites W1986163712 @default.
• W2418080963 cites W1986738273 @default.
• W2418080963 cites W1987197986 @default.
• W2418080963 cites W1993867049 @default.
• W2418080963 cites W1994671833 @default.
• W2418080963 cites W1995626628 @default.
• W2418080963 cites W2004557233 @default.
• W2418080963 cites W2005796639 @default.
• W2418080963 cites W2009352072 @default.
• W2418080963 cites W2010328731 @default.
• W2418080963 cites W2014678453 @default.
• W2418080963 cites W2015127589 @default.
• W2418080963 cites W2017100570 @default.
• W2418080963 cites W2018657673 @default.
• W2418080963 cites W2023056656 @default.
• W2418080963 cites W2024297548 @default.
• W2418080963 cites W2025105301 @default.
• W2418080963 cites W2025304087 @default.
• W2418080963 cites W2025458316 @default.
• W2418080963 cites W2026694896 @default.
• W2418080963 cites W2028398011 @default.
• W2418080963 cites W2028626541 @default.
• W2418080963 cites W2029231021 @default.
• W2418080963 cites W2029965202 @default.
• W2418080963 cites W2031539306 @default.
• W2418080963 cites W2031826267 @default.
• W2418080963 cites W2034974550 @default.
• W2418080963 cites W2039189525 @default.
• W2418080963 cites W2039461358 @default.
• W2418080963 cites W2039727350 @default.
• W2418080963 cites W2041537888 @default.
• W2418080963 cites W2042561599 @default.
• W2418080963 cites W2043279355 @default.
• W2418080963 cites W2044872435 @default.
• W2418080963 cites W2047156688 @default.
• W2418080963 cites W2054227128 @default.
• W2418080963 cites W2055523095 @default.
• W2418080963 cites W2057589371 @default.
• W2418080963 cites W2057724609 @default.
• W2418080963 cites W2059302115 @default.
• W2418080963 cites W2060050893 @default.
• W2418080963 cites W2067342622 @default.
• W2418080963 cites W2071125282 @default.
• W2418080963 cites W2071864147 @default.
• W2418080963 cites W2073424199 @default.
• W2418080963 cites W2080189336 @default.
• W2418080963 cites W2082295831 @default.
• W2418080963 cites W2082361697 @default.
• W2418080963 cites W2083269071 @default.
• W2418080963 cites W2083576610 @default.
• W2418080963 cites W2084830951 @default.
• W2418080963 cites W2090135680 @default.
• W2418080963 cites W2095044009 @default.
• W2418080963 cites W2095736123 @default.
• W2418080963 cites W2100514692 @default.
• W2418080963 cites W2102080842 @default.
• W2418080963 cites W2109329782 @default.
• W2418080963 cites W2109401568 @default.
• W2418080963 cites W2110709935 @default.
• W2418080963 cites W2113686234 @default.
• W2418080963 cites W2120069867 @default.
• W2418080963 cites W2122594969 @default.
• W2418080963 cites W2123709957 @default.
• W2418080963 cites W2124924585 @default.

• next