FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3149794663> ?p ?o ?g. }

• W3149794663 endingPage "324" @default.
• W3149794663 startingPage "304" @default.
• W3149794663 abstract "We characterize the conditional distributions of the HI gas-to-stellar mass ratio, $R_{HI}equiv M_{HI}/M_{ast}$, given the stellar mass, $M_{ast}$, of local galaxies from $M_{ast}sim 10^7$ to $10^{12}$ $M_{odot}$ separated into centrals and satellites as well as into late- and early-type galaxies (LTGs and ETGs, respectively). To do so, we use (1) the homogeneous eXtended GALEX Arecibo SDSS Survey, xGASS (Catinella et al. 2018), by re-estimating their upper limits and taking into account them in our statistical analysis; and (2) the results from a large compilation of HI data reported in Calette et al. (2018). We use the $R_{HI}$ conditional distributions combined with the Galaxy Stellar Mass Function to infer the bivariate $M_{HI}$ and $M_{ast}$ distribution of all galaxies as well of the late/early-type and central/satellite subsamples and their combinations. Satellites are on average less HI gas-rich than centrals at low and intermediate masses, with differences being larger for ETGs than LTGs; at $M_{ast}>3-5times 10^{10}$ $M_{odot}$ the differences are negligible. The differences in the HI gas content are much larger between LTGs and ETGs than between centrals and satellites. Our empirical HI Mass Function is strongly dominated by central galaxies at all masses. The empirically constrained bivariate $M_{HI}$ and $M_{ast}$ distributions presented here can be used to compare and constrain theoretical predictions as well as to generate galaxy mock catalogues." @default.
• W3149794663 created "2021-04-13" @default.
• W3149794663 creator A5025241410 @default.
• W3149794663 creator A5040010680 @default.
• W3149794663 creator A5042798740 @default.
• W3149794663 creator A5048358120 @default.
• W3149794663 creator A5060297317 @default.
• W3149794663 date "2021-05-07" @default.
• W3149794663 modified "2023-10-14" @default.
• W3149794663 title "The H <scp>i</scp> and stellar mass bivariate distribution of centrals and satellites for all, late-, and early-type local galaxies" @default.
• W3149794663 cites W1609444141 @default.
• W3149794663 cites W1632875404 @default.
• W3149794663 cites W1786379693 @default.
• W3149794663 cites W1915403329 @default.
• W3149794663 cites W1969506103 @default.
• W3149794663 cites W1987522415 @default.
• W3149794663 cites W1988235022 @default.
• W3149794663 cites W1991024873 @default.
• W3149794663 cites W1991471447 @default.
• W3149794663 cites W1991610844 @default.
• W3149794663 cites W1993114479 @default.
• W3149794663 cites W1996537612 @default.
• W3149794663 cites W1997201902 @default.
• W3149794663 cites W2000444334 @default.
• W3149794663 cites W2005796639 @default.
• W3149794663 cites W2024519938 @default.
• W3149794663 cites W2024691091 @default.
• W3149794663 cites W2030645675 @default.
• W3149794663 cites W2040093099 @default.
• W3149794663 cites W2041561966 @default.
• W3149794663 cites W2060923225 @default.
• W3149794663 cites W2064921519 @default.
• W3149794663 cites W2073501758 @default.
• W3149794663 cites W2084775077 @default.
• W3149794663 cites W2098000362 @default.
• W3149794663 cites W2103612329 @default.
• W3149794663 cites W2107779776 @default.
• W3149794663 cites W2115468377 @default.
• W3149794663 cites W2123164015 @default.
• W3149794663 cites W2124182534 @default.
• W3149794663 cites W2124199755 @default.
• W3149794663 cites W2125546908 @default.
• W3149794663 cites W2136623067 @default.
• W3149794663 cites W2140834585 @default.
• W3149794663 cites W2143498156 @default.
• W3149794663 cites W2150989398 @default.
• W3149794663 cites W2165003596 @default.
• W3149794663 cites W2173961484 @default.
• W3149794663 cites W2174907838 @default.
• W3149794663 cites W2467658441 @default.
• W3149794663 cites W2512296910 @default.
• W3149794663 cites W2545020124 @default.
• W3149794663 cites W2547347443 @default.
• W3149794663 cites W2578689462 @default.
• W3149794663 cites W2768455873 @default.
• W3149794663 cites W2783332169 @default.
• W3149794663 cites W2891429483 @default.
• W3149794663 cites W2896373226 @default.
• W3149794663 cites W2898522146 @default.
• W3149794663 cites W2899060896 @default.
• W3149794663 cites W2909962336 @default.
• W3149794663 cites W2979381411 @default.
• W3149794663 cites W2999086181 @default.
• W3149794663 cites W3002648117 @default.
• W3149794663 cites W3005563919 @default.
• W3149794663 cites W3094274128 @default.
• W3149794663 cites W3098394611 @default.
• W3149794663 cites W3099346888 @default.
• W3149794663 cites W3100220540 @default.
• W3149794663 cites W3100248076 @default.
• W3149794663 cites W3100401081 @default.
• W3149794663 cites W3101926670 @default.
• W3149794663 cites W3102136057 @default.
• W3149794663 cites W3103077803 @default.
• W3149794663 cites W3103426015 @default.
• W3149794663 cites W3103494666 @default.
• W3149794663 cites W3105028954 @default.
• W3149794663 cites W3105190296 @default.
• W3149794663 cites W3106484392 @default.
• W3149794663 cites W3123868910 @default.
• W3149794663 cites W3123916116 @default.
• W3149794663 cites W3125341864 @default.
• W3149794663 cites W3125651113 @default.
• W3149794663 cites W3125793999 @default.
• W3149794663 cites W4293241248 @default.
• W3149794663 cites W4296217314 @default.
• W3149794663 cites W4300719359 @default.
• W3149794663 doi "https://doi.org/10.1093/mnras/stab1282" @default.
• W3149794663 hasPublicationYear "2021" @default.
• W3149794663 type Work @default.
• W3149794663 sameAs 3149794663 @default.
• W3149794663 citedByCount "5" @default.
• W3149794663 countsByYear W31497946632021 @default.
• W3149794663 countsByYear W31497946632022 @default.
• W3149794663 countsByYear W31497946632023 @default.
• W3149794663 crossrefType "journal-article" @default.
• W3149794663 hasAuthorship W3149794663A5025241410 @default.
• W3149794663 hasAuthorship W3149794663A5040010680 @default.

• next