Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100209513> ?p ?o ?g. }
- W3100209513 endingPage "177" @default.
- W3100209513 startingPage "177" @default.
- W3100209513 abstract "We have used deep GALEX observations at the infall region of the Coma cluster to measure the faintest ultraviolet (UV) luminosity functions (LFs) presented for a rich galaxy cluster thus far. The Coma UV LFs are measured to MUV = −10.5 in the GALEX FUV and NUV bands, or 3.5 mag fainter than previous studies, and reach the dwarf early-type galaxy population in Coma for the first time. The Schechter faint-end slopes (α ≈ −1.39 in both GALEX bands) are shallower than reported in previous Coma UV LF studies owing to a flatter LF at faint magnitudes. A Gaussian-plus-Schechter model provides a slightly better parameterization of the UV LFs resulting in a faint-end slope of α ≈ −1.15 in both GALEX bands. The two-component model gives faint-end slopes shallower than α = −1 (a turnover) for the LFs constructed separately for passive and star-forming galaxies. The UV LFs for star-forming galaxies show a turnover at MUV ≈ −14 owing to a deficit of dwarf star-forming galaxies in Coma with stellar masses below M* = 108 M☉. A similar turnover is identified in recent UV LFs measured for the Virgo cluster suggesting this may be a common feature of local galaxy clusters, whereas the field UV LFs continue to rise at faint magnitudes. We did not identify an excess of passive galaxies as would be expected if the missing dwarf star-forming galaxies were quenched inside the cluster. In fact, the LFs for both dwarf passive and star-forming galaxies show the same turnover at faint magnitudes. We discuss the possible origin of the missing dwarf star-forming galaxies in Coma and their expected properties based on comparisons to local field galaxies." @default.
- W3100209513 created "2020-11-23" @default.
- W3100209513 creator A5030391658 @default.
- W3100209513 creator A5032135229 @default.
- W3100209513 creator A5035495817 @default.
- W3100209513 creator A5037028059 @default.
- W3100209513 creator A5042305541 @default.
- W3100209513 creator A5044374924 @default.
- W3100209513 creator A5047376847 @default.
- W3100209513 creator A5073784409 @default.
- W3100209513 date "2012-01-17" @default.
- W3100209513 modified "2023-10-02" @default.
- W3100209513 title "DEEP ULTRAVIOLET LUMINOSITY FUNCTIONS AT THE INFALL REGION OF THE COMA CLUSTER" @default.
- W3100209513 cites W1609444141 @default.
- W3100209513 cites W1662593333 @default.
- W3100209513 cites W1873415510 @default.
- W3100209513 cites W1916237623 @default.
- W3100209513 cites W1966491705 @default.
- W3100209513 cites W1966928945 @default.
- W3100209513 cites W1967290904 @default.
- W3100209513 cites W1967864402 @default.
- W3100209513 cites W1973308053 @default.
- W3100209513 cites W1975458826 @default.
- W3100209513 cites W1975485972 @default.
- W3100209513 cites W1977532327 @default.
- W3100209513 cites W1987592311 @default.
- W3100209513 cites W1989671903 @default.
- W3100209513 cites W1991294784 @default.
- W3100209513 cites W1994047004 @default.
- W3100209513 cites W1994145175 @default.
- W3100209513 cites W1994250953 @default.
- W3100209513 cites W1995715031 @default.
- W3100209513 cites W2004115979 @default.
- W3100209513 cites W2007325934 @default.
- W3100209513 cites W2007573521 @default.
- W3100209513 cites W2011029693 @default.
- W3100209513 cites W2012484998 @default.
- W3100209513 cites W2021918512 @default.
- W3100209513 cites W2024297548 @default.
- W3100209513 cites W2024674795 @default.
- W3100209513 cites W2024845050 @default.
- W3100209513 cites W2024956465 @default.
- W3100209513 cites W2028093813 @default.
- W3100209513 cites W2028715663 @default.
- W3100209513 cites W2030094391 @default.
- W3100209513 cites W2031042534 @default.
- W3100209513 cites W2032065082 @default.
- W3100209513 cites W2032792532 @default.
- W3100209513 cites W2033235483 @default.
- W3100209513 cites W2033731878 @default.
- W3100209513 cites W2034660746 @default.
- W3100209513 cites W2035387640 @default.
- W3100209513 cites W2037209838 @default.
- W3100209513 cites W2039138278 @default.
- W3100209513 cites W2039833992 @default.
- W3100209513 cites W2040405503 @default.
- W3100209513 cites W2045322559 @default.
- W3100209513 cites W2046149262 @default.
- W3100209513 cites W2053198682 @default.
- W3100209513 cites W2054131667 @default.
- W3100209513 cites W2073050616 @default.
- W3100209513 cites W2078257430 @default.
- W3100209513 cites W2082735313 @default.
- W3100209513 cites W2084741504 @default.
- W3100209513 cites W2086179169 @default.
- W3100209513 cites W2086649316 @default.
- W3100209513 cites W2088881638 @default.
- W3100209513 cites W2093671563 @default.
- W3100209513 cites W2108015652 @default.
- W3100209513 cites W2108617972 @default.
- W3100209513 cites W2111841752 @default.
- W3100209513 cites W2112172599 @default.
- W3100209513 cites W2115659244 @default.
- W3100209513 cites W2115859369 @default.
- W3100209513 cites W2116466430 @default.
- W3100209513 cites W2120361995 @default.
- W3100209513 cites W2124324031 @default.
- W3100209513 cites W2124808710 @default.
- W3100209513 cites W2125621035 @default.
- W3100209513 cites W2126688676 @default.
- W3100209513 cites W2126877617 @default.
- W3100209513 cites W2137043067 @default.
- W3100209513 cites W2140887005 @default.
- W3100209513 cites W2145679541 @default.
- W3100209513 cites W2151296334 @default.
- W3100209513 cites W2151497515 @default.
- W3100209513 cites W2153463356 @default.
- W3100209513 cites W2153554447 @default.
- W3100209513 cites W2154693853 @default.
- W3100209513 cites W2160197565 @default.
- W3100209513 cites W2162290847 @default.
- W3100209513 cites W2166365370 @default.
- W3100209513 cites W2170689655 @default.
- W3100209513 cites W2173961484 @default.
- W3100209513 cites W2951522352 @default.
- W3100209513 cites W3098160327 @default.
- W3100209513 cites W3098417747 @default.
- W3100209513 cites W3098780593 @default.