FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2901284481> ?p ?o ?g. }

• W2901284481 endingPage "617" @default.
• W2901284481 startingPage "595" @default.
• W2901284481 abstract "Minor mergers are thought to be responsible for the size growth of quiescent field galaxies with decreasing redshift. We test this hypothesis using the cluster environment as a laboratory. Satellite galaxies in clusters move at high velocities, making mergers between them rare. The stellar mass-size relation in ten clusters and in the field is measured and compared at $z~mathtt{sim}~1$. Our cluster sample contains 344 spectroscopically-confirmed cluster members with Gemini/GMOS and 182 confirmed with HST WFC3 G141 grism spectroscopy. On average, quiescent and star-forming cluster galaxies are smaller than their field counterparts by ($0.08pm0.04$) dex and ($0.07pm0.01$) dex respectively. These size offsets are consistent with the average sizes of quiescent and star-forming field galaxies between $1.2leqslant zleqslant1.5$, implying the cluster environment has inhibited size growth between this period and $z~mathtt{sim}~1$. The negligible differences measured between the $z~mathtt{sim}~0$ field and cluster quiescent mass-size relations in other works imply that the average size of quiescent cluster galaxies must rise with decreasing redshift. Using a toy model, we show that the disappearance of the compact cluster galaxies might be explained if, on average, $mathtt{sim}40%$ of them merge with their brightest cluster galaxies (BCGs) and $mathtt{sim}60%$ are tidally destroyed into the intra-cluster light (ICL) between $0leqslant zleqslant1$. This is in agreement with the observed stellar mass growth of BCGs between $0leqslant zleqslant1$ and the observed ICL stellar mass fraction at $z~mathtt{sim}~0$. Our results support minor mergers as the cause for the size growth in quiescent field galaxies, with cluster-specific processes responsible for the similarity between the field and cluster quiescent mass-size relations at low redshift." @default.
• W2901284481 created "2018-11-29" @default.
• W2901284481 creator A5007056232 @default.
• W2901284481 creator A5008236408 @default.
• W2901284481 creator A5009681773 @default.
• W2901284481 creator A5018993806 @default.
• W2901284481 creator A5021395641 @default.
• W2901284481 creator A5024842870 @default.
• W2901284481 creator A5041193928 @default.
• W2901284481 creator A5046073017 @default.
• W2901284481 creator A5053017072 @default.
• W2901284481 creator A5065482928 @default.
• W2901284481 creator A5066316052 @default.
• W2901284481 creator A5071179127 @default.
• W2901284481 creator A5078101036 @default.
• W2901284481 creator A5079133544 @default.
• W2901284481 creator A5079965553 @default.
• W2901284481 creator A5082408263 @default.
• W2901284481 date "2018-12-27" @default.
• W2901284481 modified "2023-10-17" @default.
• W2901284481 title "<i>HST</i>/WFC3 grism observations of<i><b>z</b></i>∼ 1 clusters: the cluster versus field stellar mass–size relation and evidence for size growth of quiescent galaxies from minor mergers" @default.
• W2901284481 cites W1593856062 @default.
• W2901284481 cites W1842979184 @default.
• W2901284481 cites W1898645908 @default.
• W2901284481 cites W1937529881 @default.
• W2901284481 cites W1964402260 @default.
• W2901284481 cites W1979104039 @default.
• W2901284481 cites W1980992764 @default.
• W2901284481 cites W1992635601 @default.
• W2901284481 cites W2002610082 @default.
• W2901284481 cites W2003440762 @default.
• W2901284481 cites W2007325934 @default.
• W2901284481 cites W2007521584 @default.
• W2901284481 cites W2008548976 @default.
• W2901284481 cites W2011301426 @default.
• W2901284481 cites W2020019783 @default.
• W2901284481 cites W2025020969 @default.
• W2901284481 cites W2033196817 @default.
• W2901284481 cites W2033803356 @default.
• W2901284481 cites W2043261125 @default.
• W2901284481 cites W2044853985 @default.
• W2901284481 cites W2050122780 @default.
• W2901284481 cites W2052458093 @default.
• W2901284481 cites W2052755662 @default.
• W2901284481 cites W2063182335 @default.
• W2901284481 cites W2079227246 @default.
• W2901284481 cites W2084780057 @default.
• W2901284481 cites W2089191176 @default.
• W2901284481 cites W2092121483 @default.
• W2901284481 cites W2094305767 @default.
• W2901284481 cites W2110846571 @default.
• W2901284481 cites W2110974947 @default.
• W2901284481 cites W2112030812 @default.
• W2901284481 cites W2119153888 @default.
• W2901284481 cites W2120295959 @default.
• W2901284481 cites W2124922548 @default.
• W2901284481 cites W2130164698 @default.
• W2901284481 cites W2134948061 @default.
• W2901284481 cites W2135052708 @default.
• W2901284481 cites W2142238829 @default.
• W2901284481 cites W2143498156 @default.
• W2901284481 cites W2149653371 @default.
• W2901284481 cites W2149739542 @default.
• W2901284481 cites W2150107548 @default.
• W2901284481 cites W2151062050 @default.
• W2901284481 cites W2153094038 @default.
• W2901284481 cites W2155385043 @default.
• W2901284481 cites W2155705849 @default.
• W2901284481 cites W2158454843 @default.
• W2901284481 cites W2159657041 @default.
• W2901284481 cites W2161590317 @default.
• W2901284481 cites W2162399571 @default.
• W2901284481 cites W2167965398 @default.
• W2901284481 cites W2365035587 @default.
• W2901284481 cites W2404713591 @default.
• W2901284481 cites W2521388614 @default.
• W2901284481 cites W2766606513 @default.
• W2901284481 cites W2888532099 @default.
• W2901284481 cites W3022668787 @default.
• W2901284481 cites W3097976312 @default.
• W2901284481 cites W3098105699 @default.
• W2901284481 cites W3098160327 @default.
• W2901284481 cites W3098225459 @default.
• W2901284481 cites W3098242113 @default.
• W2901284481 cites W3098318161 @default.
• W2901284481 cites W3098558780 @default.
• W2901284481 cites W3098858114 @default.
• W2901284481 cites W3099267591 @default.
• W2901284481 cites W3099428116 @default.
• W2901284481 cites W3099740765 @default.
• W2901284481 cites W3100024326 @default.
• W2901284481 cites W3100522481 @default.
• W2901284481 cites W3101018959 @default.
• W2901284481 cites W3101072469 @default.
• W2901284481 cites W3101110216 @default.
• W2901284481 cites W3101347713 @default.
• W2901284481 cites W3101627308 @default.
• W2901284481 cites W3101756302 @default.

• next