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Stellar Halos from the The Dragonfly Edge-on Galaxies Survey
We present the primary results from the Dragonfly Edge-on Galaxies Survey, an exploration of the stellar halos of twelve nearby ( d < 25 Mpc) edge-on disk galaxies with the Dragonfly Telephoto Array. The edge-on orientation of these galaxies allows their stellar halos to be explored with minimal...
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Published in: | The Astrophysical journal 2022-06, Vol.932 (1), p.44 |
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creator | Gilhuly, Colleen Merritt, Allison Abraham, Roberto Danieli, Shany Lokhorst, Deborah Liu, Qing van Dokkum, Pieter Conroy, Charlie Greco, Johnny |
description | We present the primary results from the Dragonfly Edge-on Galaxies Survey, an exploration of the stellar halos of twelve nearby (
d
< 25 Mpc) edge-on disk galaxies with the Dragonfly Telephoto Array. The edge-on orientation of these galaxies allows their stellar halos to be explored with minimal obscuration by or confusion with the much brighter disk light. Galaxies in the sample span a range of stellar masses from 10
9.68
to 10
10.88
M
⊙
. We confirm that the wide range of stellar halo mass fractions previously seen for Milky Way–mass galaxies is also found among less massive spiral galaxies. The scatter in stellar halo mass fraction is large, but we do find a significant positive correlation between stellar halo mass fraction and total stellar mass when the former is measured beyond five half-mass radii. Reasonably good agreement is found with predictions from cosmological hydrodynamical simulations, although observed stellar halo fractions appear to be somewhat lower than expected from these simulations. |
doi_str_mv | 10.3847/1538-4357/ac6750 |
format | article |
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d
< 25 Mpc) edge-on disk galaxies with the Dragonfly Telephoto Array. The edge-on orientation of these galaxies allows their stellar halos to be explored with minimal obscuration by or confusion with the much brighter disk light. Galaxies in the sample span a range of stellar masses from 10
9.68
to 10
10.88
M
⊙
. We confirm that the wide range of stellar halo mass fractions previously seen for Milky Way–mass galaxies is also found among less massive spiral galaxies. The scatter in stellar halo mass fraction is large, but we do find a significant positive correlation between stellar halo mass fraction and total stellar mass when the former is measured beyond five half-mass radii. Reasonably good agreement is found with predictions from cosmological hydrodynamical simulations, although observed stellar halo fractions appear to be somewhat lower than expected from these simulations.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/ac6750</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Astrophysics ; Disk galaxies ; Galactic halos ; Galaxies ; Galaxy photometry ; Galaxy stellar halos ; Galaxy structure ; Halos ; Milky Way ; Occultation ; Spiral galaxies ; Stars & galaxies ; Stellar mass</subject><ispartof>The Astrophysical journal, 2022-06, Vol.932 (1), p.44</ispartof><rights>2022. The Author(s). Published by the American Astronomical Society.</rights><rights>2022. 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><citedby>FETCH-LOGICAL-c350t-96989733e2e90a0c4d9d5cb10481ef917d41542d8b6ee44048fbbb8007fcdcd43</citedby><cites>FETCH-LOGICAL-c350t-96989733e2e90a0c4d9d5cb10481ef917d41542d8b6ee44048fbbb8007fcdcd43</cites><orcidid>0000-0002-4542-921X ; 0000-0002-1590-8551 ; 0000-0002-8931-4684 ; 0000-0002-2406-7344 ; 0000-0002-7490-5991 ; 0000-0001-9467-7298 ; 0000-0002-1841-2252 ; 0000-0003-4970-2874 ; 0000-0002-8282-9888</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,777,781,27905,27906</link.rule.ids></links><search><creatorcontrib>Gilhuly, Colleen</creatorcontrib><creatorcontrib>Merritt, Allison</creatorcontrib><creatorcontrib>Abraham, Roberto</creatorcontrib><creatorcontrib>Danieli, Shany</creatorcontrib><creatorcontrib>Lokhorst, Deborah</creatorcontrib><creatorcontrib>Liu, Qing</creatorcontrib><creatorcontrib>van Dokkum, Pieter</creatorcontrib><creatorcontrib>Conroy, Charlie</creatorcontrib><creatorcontrib>Greco, Johnny</creatorcontrib><title>Stellar Halos from the The Dragonfly Edge-on Galaxies Survey</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>We present the primary results from the Dragonfly Edge-on Galaxies Survey, an exploration of the stellar halos of twelve nearby (
d
< 25 Mpc) edge-on disk galaxies with the Dragonfly Telephoto Array. The edge-on orientation of these galaxies allows their stellar halos to be explored with minimal obscuration by or confusion with the much brighter disk light. Galaxies in the sample span a range of stellar masses from 10
9.68
to 10
10.88
M
⊙
. We confirm that the wide range of stellar halo mass fractions previously seen for Milky Way–mass galaxies is also found among less massive spiral galaxies. The scatter in stellar halo mass fraction is large, but we do find a significant positive correlation between stellar halo mass fraction and total stellar mass when the former is measured beyond five half-mass radii. 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d
< 25 Mpc) edge-on disk galaxies with the Dragonfly Telephoto Array. The edge-on orientation of these galaxies allows their stellar halos to be explored with minimal obscuration by or confusion with the much brighter disk light. Galaxies in the sample span a range of stellar masses from 10
9.68
to 10
10.88
M
⊙
. We confirm that the wide range of stellar halo mass fractions previously seen for Milky Way–mass galaxies is also found among less massive spiral galaxies. The scatter in stellar halo mass fraction is large, but we do find a significant positive correlation between stellar halo mass fraction and total stellar mass when the former is measured beyond five half-mass radii. Reasonably good agreement is found with predictions from cosmological hydrodynamical simulations, although observed stellar halo fractions appear to be somewhat lower than expected from these simulations.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/ac6750</doi><tpages>41</tpages><orcidid>https://orcid.org/0000-0002-4542-921X</orcidid><orcidid>https://orcid.org/0000-0002-1590-8551</orcidid><orcidid>https://orcid.org/0000-0002-8931-4684</orcidid><orcidid>https://orcid.org/0000-0002-2406-7344</orcidid><orcidid>https://orcid.org/0000-0002-7490-5991</orcidid><orcidid>https://orcid.org/0000-0001-9467-7298</orcidid><orcidid>https://orcid.org/0000-0002-1841-2252</orcidid><orcidid>https://orcid.org/0000-0003-4970-2874</orcidid><orcidid>https://orcid.org/0000-0002-8282-9888</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Astrophysics Disk galaxies Galactic halos Galaxies Galaxy photometry Galaxy stellar halos Galaxy structure Halos Milky Way Occultation Spiral galaxies Stars & galaxies Stellar mass |
title | Stellar Halos from the The Dragonfly Edge-on Galaxies Survey |
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