Loading…

Vertical Phase Mixing across the Galactic Disk

By combining the Large Sky Area Multi-object Fiber Spectroscopic Telescope and Gaia data, we investigate the vertical phase mixing across the Galactic disk. Our results confirm the existence of phase space snail shells (or phase spirals) from 6–12 kpc. We find that grouping stars by the guiding radi...

Full description

Saved in:
Bibliographic Details
Published in:The Astrophysical journal 2021-04, Vol.911 (2), p.107
Main Author: Li, Zhao-Yu
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c380t-eb43a67f79cc2c95e5c483c6ad4f03eb5ea895096356a669187642f23ba8af813
cites cdi_FETCH-LOGICAL-c380t-eb43a67f79cc2c95e5c483c6ad4f03eb5ea895096356a669187642f23ba8af813
container_end_page
container_issue 2
container_start_page 107
container_title The Astrophysical journal
container_volume 911
creator Li, Zhao-Yu
description By combining the Large Sky Area Multi-object Fiber Spectroscopic Telescope and Gaia data, we investigate the vertical phase mixing across the Galactic disk. Our results confirm the existence of phase space snail shells (or phase spirals) from 6–12 kpc. We find that grouping stars by the guiding radius ( R g ), instead of the present radius ( R ), further enhances the snail shell signal in the following aspects: (1) clarity of the snail shell shape is increased; (2) more wraps of the snail shell can be seen; (3) the phase spaces are less affected by the lack of stars closer to the disk midplane due to extinction; and (4) the phase space snail shell is amplified in greater radial ranges. Compared to the R -based snail shell, the quantitatively measured shapes are similar, except that the R g -based snail shells show more wraps with a better contrast. These lines of evidence lead to the conclusion that the guiding radius (angular momentum) is a fundamental parameter tracing the phase space snail shell across the Galactic disk. Results of our test particle simulations with impulse approximation verify that particles grouped according to R g reveal well-defined and sharper snail shell features. By comparing the radial profiles of the snail shell pitch angle between the observation and simulation, the external perturbation can be constrained to ∼500−700 Myr ago. For future vertical phase mixing study, it is recommended to use the guiding radius with additional constraints on orbital hotness (ellipticity) to improve the clarity of the phase snail.
doi_str_mv 10.3847/1538-4357/abea17
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2518770466</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2518770466</sourcerecordid><originalsourceid>FETCH-LOGICAL-c380t-eb43a67f79cc2c95e5c483c6ad4f03eb5ea895096356a669187642f23ba8af813</originalsourceid><addsrcrecordid>eNp9kE1Lw0AQhhdRMFbvHgPizbS72e-j1FqFih5UvC2T7a5NrE3cTUH_vYkRvYinYYbnnRkehI4JHlPF5IRwqjJGuZxA4YDIHZT8jHZRgjFmmaDyaR8dxFj1ba51gsaPLrSlhXV6t4Lo0pvyvdw8p2BDHWParlw6hzXYDkkvyvhyiPY8rKM7-q4j9HA5u59eZYvb-fX0fJFZqnCbuYJRENJLbW1uNXfcMkWtgCXzmLqCO1CaYy0oFyCEJkoKlvucFqDAK0JH6GTY24T6betia6p6GzbdSZPzjpaYCdFReKC-vg3OmyaUrxA-DMGmt2J6BaZXYAYrXeRsiJR187vzH_z0DxyaymhCTN4FpWmWnn4CellufA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2518770466</pqid></control><display><type>article</type><title>Vertical Phase Mixing across the Galactic Disk</title><source>In der EZB frei verfügbare Zeitschriften</source><creator>Li, Zhao-Yu</creator><creatorcontrib>Li, Zhao-Yu</creatorcontrib><description>By combining the Large Sky Area Multi-object Fiber Spectroscopic Telescope and Gaia data, we investigate the vertical phase mixing across the Galactic disk. Our results confirm the existence of phase space snail shells (or phase spirals) from 6–12 kpc. We find that grouping stars by the guiding radius ( R g ), instead of the present radius ( R ), further enhances the snail shell signal in the following aspects: (1) clarity of the snail shell shape is increased; (2) more wraps of the snail shell can be seen; (3) the phase spaces are less affected by the lack of stars closer to the disk midplane due to extinction; and (4) the phase space snail shell is amplified in greater radial ranges. Compared to the R -based snail shell, the quantitatively measured shapes are similar, except that the R g -based snail shells show more wraps with a better contrast. These lines of evidence lead to the conclusion that the guiding radius (angular momentum) is a fundamental parameter tracing the phase space snail shell across the Galactic disk. Results of our test particle simulations with impulse approximation verify that particles grouped according to R g reveal well-defined and sharper snail shell features. By comparing the radial profiles of the snail shell pitch angle between the observation and simulation, the external perturbation can be constrained to ∼500−700 Myr ago. For future vertical phase mixing study, it is recommended to use the guiding radius with additional constraints on orbital hotness (ellipticity) to improve the clarity of the phase snail.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/abea17</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Angular momentum ; Astrophysics ; Clarity ; Constraints ; Ellipticity ; Galactic disk ; Milky Way disk ; Milky Way dynamics ; Milky Way evolution ; Milky Way Galaxy ; Perturbation ; Pitch (inclination) ; Spectroscopic telescopes ; Spirals</subject><ispartof>The Astrophysical journal, 2021-04, Vol.911 (2), p.107</ispartof><rights>2021. The Author(s). Published by the American Astronomical Society.</rights><rights>Copyright IOP Publishing Apr 01, 2021</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c380t-eb43a67f79cc2c95e5c483c6ad4f03eb5ea895096356a669187642f23ba8af813</citedby><cites>FETCH-LOGICAL-c380t-eb43a67f79cc2c95e5c483c6ad4f03eb5ea895096356a669187642f23ba8af813</cites><orcidid>0000-0001-5017-7021</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail></links><search><creatorcontrib>Li, Zhao-Yu</creatorcontrib><title>Vertical Phase Mixing across the Galactic Disk</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>By combining the Large Sky Area Multi-object Fiber Spectroscopic Telescope and Gaia data, we investigate the vertical phase mixing across the Galactic disk. Our results confirm the existence of phase space snail shells (or phase spirals) from 6–12 kpc. We find that grouping stars by the guiding radius ( R g ), instead of the present radius ( R ), further enhances the snail shell signal in the following aspects: (1) clarity of the snail shell shape is increased; (2) more wraps of the snail shell can be seen; (3) the phase spaces are less affected by the lack of stars closer to the disk midplane due to extinction; and (4) the phase space snail shell is amplified in greater radial ranges. Compared to the R -based snail shell, the quantitatively measured shapes are similar, except that the R g -based snail shells show more wraps with a better contrast. These lines of evidence lead to the conclusion that the guiding radius (angular momentum) is a fundamental parameter tracing the phase space snail shell across the Galactic disk. Results of our test particle simulations with impulse approximation verify that particles grouped according to R g reveal well-defined and sharper snail shell features. By comparing the radial profiles of the snail shell pitch angle between the observation and simulation, the external perturbation can be constrained to ∼500−700 Myr ago. For future vertical phase mixing study, it is recommended to use the guiding radius with additional constraints on orbital hotness (ellipticity) to improve the clarity of the phase snail.</description><subject>Angular momentum</subject><subject>Astrophysics</subject><subject>Clarity</subject><subject>Constraints</subject><subject>Ellipticity</subject><subject>Galactic disk</subject><subject>Milky Way disk</subject><subject>Milky Way dynamics</subject><subject>Milky Way evolution</subject><subject>Milky Way Galaxy</subject><subject>Perturbation</subject><subject>Pitch (inclination)</subject><subject>Spectroscopic telescopes</subject><subject>Spirals</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNp9kE1Lw0AQhhdRMFbvHgPizbS72e-j1FqFih5UvC2T7a5NrE3cTUH_vYkRvYinYYbnnRkehI4JHlPF5IRwqjJGuZxA4YDIHZT8jHZRgjFmmaDyaR8dxFj1ba51gsaPLrSlhXV6t4Lo0pvyvdw8p2BDHWParlw6hzXYDkkvyvhyiPY8rKM7-q4j9HA5u59eZYvb-fX0fJFZqnCbuYJRENJLbW1uNXfcMkWtgCXzmLqCO1CaYy0oFyCEJkoKlvucFqDAK0JH6GTY24T6betia6p6GzbdSZPzjpaYCdFReKC-vg3OmyaUrxA-DMGmt2J6BaZXYAYrXeRsiJR187vzH_z0DxyaymhCTN4FpWmWnn4CellufA</recordid><startdate>20210401</startdate><enddate>20210401</enddate><creator>Li, Zhao-Yu</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/0000-0001-5017-7021</orcidid></search><sort><creationdate>20210401</creationdate><title>Vertical Phase Mixing across the Galactic Disk</title><author>Li, Zhao-Yu</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c380t-eb43a67f79cc2c95e5c483c6ad4f03eb5ea895096356a669187642f23ba8af813</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Angular momentum</topic><topic>Astrophysics</topic><topic>Clarity</topic><topic>Constraints</topic><topic>Ellipticity</topic><topic>Galactic disk</topic><topic>Milky Way disk</topic><topic>Milky Way dynamics</topic><topic>Milky Way evolution</topic><topic>Milky Way Galaxy</topic><topic>Perturbation</topic><topic>Pitch (inclination)</topic><topic>Spectroscopic telescopes</topic><topic>Spirals</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Li, Zhao-Yu</creatorcontrib><collection>IOP Publishing Free Content</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>Li, Zhao-Yu</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Vertical Phase Mixing across the Galactic Disk</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2021-04-01</date><risdate>2021</risdate><volume>911</volume><issue>2</issue><spage>107</spage><pages>107-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>By combining the Large Sky Area Multi-object Fiber Spectroscopic Telescope and Gaia data, we investigate the vertical phase mixing across the Galactic disk. Our results confirm the existence of phase space snail shells (or phase spirals) from 6–12 kpc. We find that grouping stars by the guiding radius ( R g ), instead of the present radius ( R ), further enhances the snail shell signal in the following aspects: (1) clarity of the snail shell shape is increased; (2) more wraps of the snail shell can be seen; (3) the phase spaces are less affected by the lack of stars closer to the disk midplane due to extinction; and (4) the phase space snail shell is amplified in greater radial ranges. Compared to the R -based snail shell, the quantitatively measured shapes are similar, except that the R g -based snail shells show more wraps with a better contrast. These lines of evidence lead to the conclusion that the guiding radius (angular momentum) is a fundamental parameter tracing the phase space snail shell across the Galactic disk. Results of our test particle simulations with impulse approximation verify that particles grouped according to R g reveal well-defined and sharper snail shell features. By comparing the radial profiles of the snail shell pitch angle between the observation and simulation, the external perturbation can be constrained to ∼500−700 Myr ago. For future vertical phase mixing study, it is recommended to use the guiding radius with additional constraints on orbital hotness (ellipticity) to improve the clarity of the phase snail.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/abea17</doi><tpages>27</tpages><orcidid>https://orcid.org/0000-0001-5017-7021</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2021-04, Vol.911 (2), p.107
issn 0004-637X
1538-4357
language eng
recordid cdi_proquest_journals_2518770466
source In der EZB frei verfügbare Zeitschriften
subjects Angular momentum
Astrophysics
Clarity
Constraints
Ellipticity
Galactic disk
Milky Way disk
Milky Way dynamics
Milky Way evolution
Milky Way Galaxy
Perturbation
Pitch (inclination)
Spectroscopic telescopes
Spirals
title Vertical Phase Mixing across the Galactic Disk
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-03-06T12%3A47%3A56IST&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=Vertical%20Phase%20Mixing%20across%20the%20Galactic%20Disk&rft.jtitle=The%20Astrophysical%20journal&rft.au=Li,%20Zhao-Yu&rft.date=2021-04-01&rft.volume=911&rft.issue=2&rft.spage=107&rft.pages=107-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/abea17&rft_dat=%3Cproquest_cross%3E2518770466%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c380t-eb43a67f79cc2c95e5c483c6ad4f03eb5ea895096356a669187642f23ba8af813%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2518770466&rft_id=info:pmid/&rfr_iscdi=true