Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations

Solar-like oscillations have been detected in thousands of stars thanks to modern space missions. These oscillations have been used to measure stellar masses and ages, which have been widely applied in Galactic archeology. One of the pillars of such applications is the ν max scaling relation: the fr...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2024-02, Vol.962 (2), p.118
Hauptverfasser: Zhou, Yixiao, Christensen-Dalsgaard, Jørgen, Asplund, Martin, Li, Yaguang, Trampedach, Regner, Ting, Yuan-Sen, Rørsted, Jakob L.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 2
container_start_page 118
container_title The Astrophysical journal
container_volume 962
creator Zhou, Yixiao
Christensen-Dalsgaard, Jørgen
Asplund, Martin
Li, Yaguang
Trampedach, Regner
Ting, Yuan-Sen
Rørsted, Jakob L.
description Solar-like oscillations have been detected in thousands of stars thanks to modern space missions. These oscillations have been used to measure stellar masses and ages, which have been widely applied in Galactic archeology. One of the pillars of such applications is the ν max scaling relation: the frequency of maximum power ν max , assumed to be proportional to the acoustic cutoff frequency, ν ac , scales with effective temperature and surface gravity. However, the theoretical basis of the ν max scaling relation is uncertain, and there is an ongoing debate about whether it can be applied to metal-poor stars. We investigate the metallicity dependence of the ν max scaling relation by carrying out 3D near-surface convection simulations for solar-type stars with [Fe/H] between −3 and 0.5 dex. First, we found a negative correlation between ν ac and metallicity from the 3D models. This is in tension with the positive correlation identified by studies using 1D models. Second, we estimated theoretical ν max values using velocity amplitudes determined from first principles, by quantifying the mode excitation and damping rates with methods validated in our previous works. We found that  ν max does not show correlation with metallicity at solar effective temperature and surface gravity. This study opens an exciting prospect of testing the asteroseismic scaling relations against realistic 3D hydrodynamical stellar models.
doi_str_mv 10.3847/1538-4357/ad1834
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2926187194</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2926187194</sourcerecordid><originalsourceid>FETCH-LOGICAL-c303t-5d493e1b77f0319127f5324e2bc7efd5e80b19e0b95bd7e5198112cbaba06b403</originalsourceid><addsrcrecordid>eNp1kN9KwzAUh4MoOKf3Xga8tS5p0qW5EtmmDiaCU_DKkLSnW0bb1KYT93C-gs9ka0WvvDp_-H3nwIfQKSUXLOZiRCMWB5xFYqRTGjO-hwa_q300IITwYMzE8yE68n7TjaGUA_QydeBxswb8-VHod7xMdG7LFX6AXDfWlXgKFZQpbrs7aHSe28Q2u0s8L71drRuPs9oVmE3xxJVvkHwjS1tse9ofo4NM5x5OfuoQPV3PHie3weL-Zj65WgQJI6wJopRLBtQIkRFGJQ1FFrGQQ2gSAVkaQUwMlUCMjEwqIKIypjRMjDaajA0nbIjO-rtV7V634Bu1cdu6bF-qUIZjGgsqeZsifSqpnfc1ZKqqbaHrnaJEdRZVp0x1ylRvsUXOe8S66u_mv_EvVv9zQQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2926187194</pqid></control><display><type>article</type><title>Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations</title><source>DOAJ Directory of Open Access Journals</source><source>Institute of Physics Open Access Journal Titles</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Zhou, Yixiao ; Christensen-Dalsgaard, Jørgen ; Asplund, Martin ; Li, Yaguang ; Trampedach, Regner ; Ting, Yuan-Sen ; Rørsted, Jakob L.</creator><creatorcontrib>Zhou, Yixiao ; Christensen-Dalsgaard, Jørgen ; Asplund, Martin ; Li, Yaguang ; Trampedach, Regner ; Ting, Yuan-Sen ; Rørsted, Jakob L.</creatorcontrib><description>Solar-like oscillations have been detected in thousands of stars thanks to modern space missions. These oscillations have been used to measure stellar masses and ages, which have been widely applied in Galactic archeology. One of the pillars of such applications is the ν max scaling relation: the frequency of maximum power ν max , assumed to be proportional to the acoustic cutoff frequency, ν ac , scales with effective temperature and surface gravity. However, the theoretical basis of the ν max scaling relation is uncertain, and there is an ongoing debate about whether it can be applied to metal-poor stars. We investigate the metallicity dependence of the ν max scaling relation by carrying out 3D near-surface convection simulations for solar-type stars with [Fe/H] between −3 and 0.5 dex. First, we found a negative correlation between ν ac and metallicity from the 3D models. This is in tension with the positive correlation identified by studies using 1D models. Second, we estimated theoretical ν max values using velocity amplitudes determined from first principles, by quantifying the mode excitation and damping rates with methods validated in our previous works. We found that  ν max does not show correlation with metallicity at solar effective temperature and surface gravity. This study opens an exciting prospect of testing the asteroseismic scaling relations against realistic 3D hydrodynamical stellar models.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/ad1834</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Archaeology ; Astronomical models ; Convection ; Correlation ; Damping ; First principles ; Maximum power ; Metallicity ; One dimensional models ; Oscillations ; Pulsation modes ; Radiative magnetohydrodynamics ; Scaling ; Solar oscillations ; Space missions ; Stars ; Stellar atmospheres ; Stellar convection envelopes ; Stellar models ; Stellar oscillations ; Stellar seismology ; Three dimensional models</subject><ispartof>The Astrophysical journal, 2024-02, Vol.962 (2), p.118</ispartof><rights>2024. The Author(s). Published by the American Astronomical Society.</rights><rights>2024. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c303t-5d493e1b77f0319127f5324e2bc7efd5e80b19e0b95bd7e5198112cbaba06b403</cites><orcidid>0000-0003-3020-4437 ; 0000-0001-5137-0966 ; 0000-0001-5082-9536 ; 0000-0003-0817-6126 ; 0000-0003-0866-6141</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/ad1834/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>314,780,784,864,27924,27925,38890,53867</link.rule.ids></links><search><creatorcontrib>Zhou, Yixiao</creatorcontrib><creatorcontrib>Christensen-Dalsgaard, Jørgen</creatorcontrib><creatorcontrib>Asplund, Martin</creatorcontrib><creatorcontrib>Li, Yaguang</creatorcontrib><creatorcontrib>Trampedach, Regner</creatorcontrib><creatorcontrib>Ting, Yuan-Sen</creatorcontrib><creatorcontrib>Rørsted, Jakob L.</creatorcontrib><title>Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>Solar-like oscillations have been detected in thousands of stars thanks to modern space missions. These oscillations have been used to measure stellar masses and ages, which have been widely applied in Galactic archeology. One of the pillars of such applications is the ν max scaling relation: the frequency of maximum power ν max , assumed to be proportional to the acoustic cutoff frequency, ν ac , scales with effective temperature and surface gravity. However, the theoretical basis of the ν max scaling relation is uncertain, and there is an ongoing debate about whether it can be applied to metal-poor stars. We investigate the metallicity dependence of the ν max scaling relation by carrying out 3D near-surface convection simulations for solar-type stars with [Fe/H] between −3 and 0.5 dex. First, we found a negative correlation between ν ac and metallicity from the 3D models. This is in tension with the positive correlation identified by studies using 1D models. Second, we estimated theoretical ν max values using velocity amplitudes determined from first principles, by quantifying the mode excitation and damping rates with methods validated in our previous works. We found that  ν max does not show correlation with metallicity at solar effective temperature and surface gravity. This study opens an exciting prospect of testing the asteroseismic scaling relations against realistic 3D hydrodynamical stellar models.</description><subject>Archaeology</subject><subject>Astronomical models</subject><subject>Convection</subject><subject>Correlation</subject><subject>Damping</subject><subject>First principles</subject><subject>Maximum power</subject><subject>Metallicity</subject><subject>One dimensional models</subject><subject>Oscillations</subject><subject>Pulsation modes</subject><subject>Radiative magnetohydrodynamics</subject><subject>Scaling</subject><subject>Solar oscillations</subject><subject>Space missions</subject><subject>Stars</subject><subject>Stellar atmospheres</subject><subject>Stellar convection envelopes</subject><subject>Stellar models</subject><subject>Stellar oscillations</subject><subject>Stellar seismology</subject><subject>Three dimensional models</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><recordid>eNp1kN9KwzAUh4MoOKf3Xga8tS5p0qW5EtmmDiaCU_DKkLSnW0bb1KYT93C-gs9ka0WvvDp_-H3nwIfQKSUXLOZiRCMWB5xFYqRTGjO-hwa_q300IITwYMzE8yE68n7TjaGUA_QydeBxswb8-VHod7xMdG7LFX6AXDfWlXgKFZQpbrs7aHSe28Q2u0s8L71drRuPs9oVmE3xxJVvkHwjS1tse9ofo4NM5x5OfuoQPV3PHie3weL-Zj65WgQJI6wJopRLBtQIkRFGJQ1FFrGQQ2gSAVkaQUwMlUCMjEwqIKIypjRMjDaajA0nbIjO-rtV7V634Bu1cdu6bF-qUIZjGgsqeZsifSqpnfc1ZKqqbaHrnaJEdRZVp0x1ylRvsUXOe8S66u_mv_EvVv9zQQ</recordid><startdate>20240201</startdate><enddate>20240201</enddate><creator>Zhou, Yixiao</creator><creator>Christensen-Dalsgaard, Jørgen</creator><creator>Asplund, Martin</creator><creator>Li, Yaguang</creator><creator>Trampedach, Regner</creator><creator>Ting, Yuan-Sen</creator><creator>Rørsted, Jakob L.</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-3020-4437</orcidid><orcidid>https://orcid.org/0000-0001-5137-0966</orcidid><orcidid>https://orcid.org/0000-0001-5082-9536</orcidid><orcidid>https://orcid.org/0000-0003-0817-6126</orcidid><orcidid>https://orcid.org/0000-0003-0866-6141</orcidid></search><sort><creationdate>20240201</creationdate><title>Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations</title><author>Zhou, Yixiao ; Christensen-Dalsgaard, Jørgen ; Asplund, Martin ; Li, Yaguang ; Trampedach, Regner ; Ting, Yuan-Sen ; Rørsted, Jakob L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c303t-5d493e1b77f0319127f5324e2bc7efd5e80b19e0b95bd7e5198112cbaba06b403</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Archaeology</topic><topic>Astronomical models</topic><topic>Convection</topic><topic>Correlation</topic><topic>Damping</topic><topic>First principles</topic><topic>Maximum power</topic><topic>Metallicity</topic><topic>One dimensional models</topic><topic>Oscillations</topic><topic>Pulsation modes</topic><topic>Radiative magnetohydrodynamics</topic><topic>Scaling</topic><topic>Solar oscillations</topic><topic>Space missions</topic><topic>Stars</topic><topic>Stellar atmospheres</topic><topic>Stellar convection envelopes</topic><topic>Stellar models</topic><topic>Stellar oscillations</topic><topic>Stellar seismology</topic><topic>Three dimensional models</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zhou, Yixiao</creatorcontrib><creatorcontrib>Christensen-Dalsgaard, Jørgen</creatorcontrib><creatorcontrib>Asplund, Martin</creatorcontrib><creatorcontrib>Li, Yaguang</creatorcontrib><creatorcontrib>Trampedach, Regner</creatorcontrib><creatorcontrib>Ting, Yuan-Sen</creatorcontrib><creatorcontrib>Rørsted, Jakob L.</creatorcontrib><collection>Institute of Physics Open Access Journal Titles</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhou, Yixiao</au><au>Christensen-Dalsgaard, Jørgen</au><au>Asplund, Martin</au><au>Li, Yaguang</au><au>Trampedach, Regner</au><au>Ting, Yuan-Sen</au><au>Rørsted, Jakob L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2024-02-01</date><risdate>2024</risdate><volume>962</volume><issue>2</issue><spage>118</spage><pages>118-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Solar-like oscillations have been detected in thousands of stars thanks to modern space missions. These oscillations have been used to measure stellar masses and ages, which have been widely applied in Galactic archeology. One of the pillars of such applications is the ν max scaling relation: the frequency of maximum power ν max , assumed to be proportional to the acoustic cutoff frequency, ν ac , scales with effective temperature and surface gravity. However, the theoretical basis of the ν max scaling relation is uncertain, and there is an ongoing debate about whether it can be applied to metal-poor stars. We investigate the metallicity dependence of the ν max scaling relation by carrying out 3D near-surface convection simulations for solar-type stars with [Fe/H] between −3 and 0.5 dex. First, we found a negative correlation between ν ac and metallicity from the 3D models. This is in tension with the positive correlation identified by studies using 1D models. Second, we estimated theoretical ν max values using velocity amplitudes determined from first principles, by quantifying the mode excitation and damping rates with methods validated in our previous works. We found that  ν max does not show correlation with metallicity at solar effective temperature and surface gravity. This study opens an exciting prospect of testing the asteroseismic scaling relations against realistic 3D hydrodynamical stellar models.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/ad1834</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0003-3020-4437</orcidid><orcidid>https://orcid.org/0000-0001-5137-0966</orcidid><orcidid>https://orcid.org/0000-0001-5082-9536</orcidid><orcidid>https://orcid.org/0000-0003-0817-6126</orcidid><orcidid>https://orcid.org/0000-0003-0866-6141</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2024-02, Vol.962 (2), p.118
issn 0004-637X
1538-4357
language eng
recordid cdi_proquest_journals_2926187194
source DOAJ Directory of Open Access Journals; Institute of Physics Open Access Journal Titles; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection
subjects Archaeology
Astronomical models
Convection
Correlation
Damping
First principles
Maximum power
Metallicity
One dimensional models
Oscillations
Pulsation modes
Radiative magnetohydrodynamics
Scaling
Solar oscillations
Space missions
Stars
Stellar atmospheres
Stellar convection envelopes
Stellar models
Stellar oscillations
Stellar seismology
Three dimensional models
title Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-24T22%3A47%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Does%20the%20%CE%BDmax%20Scaling%20Relation%20Depend%20on%20Metallicity?%20Insights%20from%203D%20Convection%20Simulations&rft.jtitle=The%20Astrophysical%20journal&rft.au=Zhou,%20Yixiao&rft.date=2024-02-01&rft.volume=962&rft.issue=2&rft.spage=118&rft.pages=118-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/ad1834&rft_dat=%3Cproquest_cross%3E2926187194%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2926187194&rft_id=info:pmid/&rfr_iscdi=true