Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100458315> ?p ?o ?g. }
- W3100458315 endingPage "80" @default.
- W3100458315 startingPage "80" @default.
- W3100458315 abstract "We select a sample of galaxies from the Sloan Digital Sky Survey Data Release 7 (SDSS-DR7) where galaxies are classified, through visual inspection, as hosting strong bars, weak bars, or as unbarred galaxies, and make use of H i mass and kinematic information from the Arecibo Legacy Fast ALFA survey catalog, to study the stellar, atomic gas, and dark matter content of barred disk galaxies. We find, in agreement with previous studies, that the bar fraction increases with increasing stellar mass. A similar trend is found with total baryonic mass, although the dependence is not as strong as with stellar mass, due to the contribution of gas. The bar fraction shows a decrease with increasing gas mass fraction. This anticorrelation between the likelihood of a galaxy hosting a bar with the gas richness of the galaxy results from the inhibiting effect the gas has in the formation of bars. We also find that for massive galaxies with stellar masses larger than 1010 M⊙, at fixed stellar mass, the bar fraction decreases with increasing global halo mass (i.e., halo mass measured up to a radius of the order of the H i disk extent)." @default.
- W3100458315 created "2020-11-23" @default.
- W3100458315 creator A5085381160 @default.
- W3100458315 date "2017-01-19" @default.
- W3100458315 modified "2023-09-30" @default.
- W3100458315 title "STELLAR, GAS, AND DARK MATTER CONTENT OF BARRED GALAXIES" @default.
- W3100458315 cites W1883767967 @default.
- W3100458315 cites W1898684449 @default.
- W3100458315 cites W1911431810 @default.
- W3100458315 cites W1973221593 @default.
- W3100458315 cites W1982735095 @default.
- W3100458315 cites W1987522415 @default.
- W3100458315 cites W1988235022 @default.
- W3100458315 cites W1989685397 @default.
- W3100458315 cites W1992212948 @default.
- W3100458315 cites W1999149150 @default.
- W3100458315 cites W2009330294 @default.
- W3100458315 cites W2014592430 @default.
- W3100458315 cites W2020844506 @default.
- W3100458315 cites W2021256493 @default.
- W3100458315 cites W2028715663 @default.
- W3100458315 cites W2032729025 @default.
- W3100458315 cites W2034040738 @default.
- W3100458315 cites W2035541286 @default.
- W3100458315 cites W2037683220 @default.
- W3100458315 cites W2039487356 @default.
- W3100458315 cites W2046301112 @default.
- W3100458315 cites W2048502077 @default.
- W3100458315 cites W2048971024 @default.
- W3100458315 cites W2050371636 @default.
- W3100458315 cites W2050660101 @default.
- W3100458315 cites W2057696957 @default.
- W3100458315 cites W2064620738 @default.
- W3100458315 cites W2066452342 @default.
- W3100458315 cites W2069360457 @default.
- W3100458315 cites W2077899319 @default.
- W3100458315 cites W2080927107 @default.
- W3100458315 cites W2084723753 @default.
- W3100458315 cites W2084775077 @default.
- W3100458315 cites W2093905654 @default.
- W3100458315 cites W2115509165 @default.
- W3100458315 cites W2118435754 @default.
- W3100458315 cites W2122680932 @default.
- W3100458315 cites W2124199755 @default.
- W3100458315 cites W2125410998 @default.
- W3100458315 cites W2128886718 @default.
- W3100458315 cites W2129802004 @default.
- W3100458315 cites W2130225077 @default.
- W3100458315 cites W2130527528 @default.
- W3100458315 cites W2136147728 @default.
- W3100458315 cites W2142918001 @default.
- W3100458315 cites W2143677751 @default.
- W3100458315 cites W2143682288 @default.
- W3100458315 cites W2144824227 @default.
- W3100458315 cites W2152498713 @default.
- W3100458315 cites W2153690020 @default.
- W3100458315 cites W2157101327 @default.
- W3100458315 cites W2165003596 @default.
- W3100458315 cites W2166365370 @default.
- W3100458315 cites W2492811461 @default.
- W3100458315 cites W2951432302 @default.
- W3100458315 cites W3098339996 @default.
- W3100458315 cites W3098429351 @default.
- W3100458315 cites W3098779512 @default.
- W3100458315 cites W3098935255 @default.
- W3100458315 cites W3099767561 @default.
- W3100458315 cites W3099888993 @default.
- W3100458315 cites W3100024326 @default.
- W3100458315 cites W3100424774 @default.
- W3100458315 cites W3100532808 @default.
- W3100458315 cites W3101423777 @default.
- W3100458315 cites W3101851245 @default.
- W3100458315 cites W3101990160 @default.
- W3100458315 cites W3102974675 @default.
- W3100458315 cites W3102981450 @default.
- W3100458315 cites W3103162296 @default.
- W3100458315 cites W3103204772 @default.
- W3100458315 cites W3103233148 @default.
- W3100458315 cites W3103868583 @default.
- W3100458315 cites W3104349085 @default.
- W3100458315 cites W3105004513 @default.
- W3100458315 cites W3105422192 @default.
- W3100458315 cites W3106271465 @default.
- W3100458315 cites W3106467243 @default.
- W3100458315 cites W3106487884 @default.
- W3100458315 cites W3121770305 @default.
- W3100458315 cites W3123278040 @default.
- W3100458315 cites W3123991250 @default.
- W3100458315 cites W4236294084 @default.
- W3100458315 cites W4298349320 @default.
- W3100458315 doi "https://doi.org/10.3847/1538-4357/835/1/80" @default.
- W3100458315 hasPublicationYear "2017" @default.
- W3100458315 type Work @default.
- W3100458315 sameAs 3100458315 @default.
- W3100458315 citedByCount "27" @default.
- W3100458315 countsByYear W31004583152017 @default.
- W3100458315 countsByYear W31004583152018 @default.
- W3100458315 countsByYear W31004583152019 @default.