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Globular Cluster — Bulge connection: Population synthesis models with multiple populations
Recent analyses of Lee et al. (2018, 2019) have confirmed that Galactic bulge consists of stellar populations originated from Milky Way globular clusters (MWGCs). Motivated by this, here we present the evolutionary population synthesis (EPS) for the Galactic bulge and early-type galaxies (ETGs) with...
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Published in: | Proceedings of the International Astronomical Union 2019-05, Vol.14 (S351), p.277-280 |
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container_end_page | 280 |
container_issue | S351 |
container_start_page | 277 |
container_title | Proceedings of the International Astronomical Union |
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creator | Chung, Chul Lee, Young-Wook Lim, Dongwook Hong, Seungsoo Kim, Jenny J. Kang, Yijung Yoon, Suk-Jin |
description | Recent analyses of Lee
et al.
(2018, 2019) have confirmed that Galactic bulge consists of stellar populations originated from Milky Way globular clusters (MWGCs). Motivated by this, here we present the evolutionary population synthesis (EPS) for the Galactic bulge and early-type galaxies (ETGs) with the realistic treatment of individual variations in light elements observed in the MWGCs. We have utilized our model with GC-origin populations to explain the CN spread observed in ETGs, and the results show remarkable matches with the observations. We further employ our model to estimate the age of ETGs, which are considered as good analogs for the MW bulge. We find that, without the effect of our new treatments, EPS models will almost always underestimate the true age of ETGs. Our analysis indicates that the EPS with GC-origin populations is an essential constraint in determining the ETG formation epoch and is closely related to understanding the evolution of the Universe. |
doi_str_mv | 10.1017/S1743921319007038 |
format | article |
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(2018, 2019) have confirmed that Galactic bulge consists of stellar populations originated from Milky Way globular clusters (MWGCs). Motivated by this, here we present the evolutionary population synthesis (EPS) for the Galactic bulge and early-type galaxies (ETGs) with the realistic treatment of individual variations in light elements observed in the MWGCs. We have utilized our model with GC-origin populations to explain the CN spread observed in ETGs, and the results show remarkable matches with the observations. We further employ our model to estimate the age of ETGs, which are considered as good analogs for the MW bulge. We find that, without the effect of our new treatments, EPS models will almost always underestimate the true age of ETGs. Our analysis indicates that the EPS with GC-origin populations is an essential constraint in determining the ETG formation epoch and is closely related to understanding the evolution of the Universe.</description><identifier>ISSN: 1743-9213</identifier><identifier>EISSN: 1743-9221</identifier><identifier>DOI: 10.1017/S1743921319007038</identifier><language>eng</language><publisher>Cambridge: Cambridge University Press</publisher><subject>Astronomical models ; Astronomy ; Celestial bodies ; Galactic bulge ; Galactic clusters ; Galactic evolution ; Galaxies ; Globular clusters ; Light elements ; Milky Way ; Stellar populations ; Synthesis</subject><ispartof>Proceedings of the International Astronomical Union, 2019-05, Vol.14 (S351), p.277-280</ispartof><rights>Copyright Cambridge University Press May 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c188t-56be656f6d6cf0a31711ad75b756da783195a2fb3e5a652d3101cdf6b66981893</citedby><cites>FETCH-LOGICAL-c188t-56be656f6d6cf0a31711ad75b756da783195a2fb3e5a652d3101cdf6b66981893</cites><orcidid>0000-0001-6812-4542</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Chung, Chul</creatorcontrib><creatorcontrib>Lee, Young-Wook</creatorcontrib><creatorcontrib>Lim, Dongwook</creatorcontrib><creatorcontrib>Hong, Seungsoo</creatorcontrib><creatorcontrib>Kim, Jenny J.</creatorcontrib><creatorcontrib>Kang, Yijung</creatorcontrib><creatorcontrib>Yoon, Suk-Jin</creatorcontrib><title>Globular Cluster — Bulge connection: Population synthesis models with multiple populations</title><title>Proceedings of the International Astronomical Union</title><description>Recent analyses of Lee
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Our analysis indicates that the EPS with GC-origin populations is an essential constraint in determining the ETG formation epoch and is closely related to understanding the evolution of the Universe.</description><subject>Astronomical models</subject><subject>Astronomy</subject><subject>Celestial bodies</subject><subject>Galactic bulge</subject><subject>Galactic clusters</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Globular clusters</subject><subject>Light elements</subject><subject>Milky Way</subject><subject>Stellar populations</subject><subject>Synthesis</subject><issn>1743-9213</issn><issn>1743-9221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNplkM1KxDAURoMoOFYfwF3AdTW3mfzUnRZnFAYU1J1Q0jZ1OqRNTVJkdj6ET-iT2DIyG1f343K4l_MhdA7kEgiIq2cQc5omQCElRBAqD9BsWsVpksDhPgM9RifebwiZc0nZDL0tjS0GoxzOzOCDdvjn6xvfDuZd49J2nS5DY7tr_GT7kZoy9tsurLVvPG5tpY3Hn01Y43YwoemNxv2e9KfoqFbG67O_GaHXxd1Ldh-vHpcP2c0qLkHKEDNeaM54zSte1kRREACqEqwQjFdKyNGJqaQuqGaKs6Sio3FZ1bzgPJUgUxqhi93d3tmPQfuQb-zguvFlnlDBBJFktI0Q7KjSWe-drvPeNa1y2xxIPpWY_yuR_gIRXWXr</recordid><startdate>20190501</startdate><enddate>20190501</enddate><creator>Chung, Chul</creator><creator>Lee, Young-Wook</creator><creator>Lim, Dongwook</creator><creator>Hong, Seungsoo</creator><creator>Kim, Jenny J.</creator><creator>Kang, Yijung</creator><creator>Yoon, Suk-Jin</creator><general>Cambridge University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope><orcidid>https://orcid.org/0000-0001-6812-4542</orcidid></search><sort><creationdate>20190501</creationdate><title>Globular Cluster — Bulge connection: Population synthesis models with multiple populations</title><author>Chung, Chul ; 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et al.
(2018, 2019) have confirmed that Galactic bulge consists of stellar populations originated from Milky Way globular clusters (MWGCs). Motivated by this, here we present the evolutionary population synthesis (EPS) for the Galactic bulge and early-type galaxies (ETGs) with the realistic treatment of individual variations in light elements observed in the MWGCs. We have utilized our model with GC-origin populations to explain the CN spread observed in ETGs, and the results show remarkable matches with the observations. We further employ our model to estimate the age of ETGs, which are considered as good analogs for the MW bulge. We find that, without the effect of our new treatments, EPS models will almost always underestimate the true age of ETGs. Our analysis indicates that the EPS with GC-origin populations is an essential constraint in determining the ETG formation epoch and is closely related to understanding the evolution of the Universe.</abstract><cop>Cambridge</cop><pub>Cambridge University Press</pub><doi>10.1017/S1743921319007038</doi><tpages>4</tpages><orcidid>https://orcid.org/0000-0001-6812-4542</orcidid></addata></record> |
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subjects | Astronomical models Astronomy Celestial bodies Galactic bulge Galactic clusters Galactic evolution Galaxies Globular clusters Light elements Milky Way Stellar populations Synthesis |
title | Globular Cluster — Bulge connection: Population synthesis models with multiple populations |
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