A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a
Here we present the Spitzer IRS spectrum of CVSO 224, the sole transitional disk located within the [image]10 Myr old 25 Orionis group in Orion OB1a. A model fit to the spectral energy distribution of this object indicates a [image]7 AU inner disk hole that contains a small amount of optically thin...
Gespeichert in:
Veröffentlicht in: | The Astrophysical journal 2008, Vol.689 (2), p.L145-L148 |
---|---|
Hauptverfasser: | , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | L148 |
---|---|
container_issue | 2 |
container_start_page | L145 |
container_title | The Astrophysical journal |
container_volume | 689 |
creator | Espaillat, C Muzerolle, J Hernández, J Briceño, C Calvet, N D’Alessio, P McClure, M Watson, D. M Hartmann, L Sargent, B |
description | Here we present the Spitzer IRS spectrum of CVSO 224, the sole transitional disk located within the [image]10 Myr old 25 Orionis group in Orion OB1a. A model fit to the spectral energy distribution of this object indicates a [image]7 AU inner disk hole that contains a small amount of optically thin dust. In previous studies, CVSO 224 had been classified as a weak-line T Tauri star based on its H alpha equivalent width, but here we find an accretion rate of 7 x 10[image] M sub([image]) yr[image] based on high- resolution Hectochelle data. CVSO 224's low [image] is in line with photoevaporative clearing theories. However, the Spitzer IRS spectrum of CVSO 224 has a substantial mid-infrared excess beyond 20 [mu]m which indicates that it is surrounded by a massive outer disk. Millimeter measurements are necessary to constrain the mass of the outer disk around CVSO 224 in order to confirm that photoevaporation is not the mechanism behind creating its inner disk hole. |
doi_str_mv | 10.1086/595869 |
format | Article |
fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_crossref_primary_10_1086_595869</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>743451673</sourcerecordid><originalsourceid>FETCH-LOGICAL-c3259-76f23e1a56fa6a00e7d53bc83e31a2fab3b74041021106d96e8c2e8ee17860d43</originalsourceid><addsrcrecordid>eNp90MtKAzEYhuEgCtaq1xAX6kJG8-c0yUao9QiVLqzrkGYyEp3O1KRFuvHandJiFcRVEnj4Ai9Ch0DOgSh5IbRQUm-hDgimMs5Evv3jvov2UnolhHCqdQdd9vBT1XxUC9xzLvpZqF_wJxD8uIhZUxV4FG2dwiw0ta3wdUhvONR4GNs3Hl6B3Uc7pa2SP1ifXfR8ezPq32eD4d1DvzfIHKNCZ7ksKfNghSyttIT4vBBs7BTzDCwt7ZiNc044EApAZKGlV4565T3kSpKCsy46Xe1OY_M-92lmJiE5X1W29s08mZwzLkDmrJUn_0rQHASlcgNdbFKKvjTTGCY2LgwQswxpViFbeLxetMnZqmyLuJC-NSVaSAG0dWcrF5rpZqvtbpbdjVTaUDMALsy0KFt99If-_fMXs0WGAA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>19415226</pqid></control><display><type>article</type><title>A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a</title><source>Institute of Physics Open Access Journal Titles</source><creator>Espaillat, C ; Muzerolle, J ; Hernández, J ; Briceño, C ; Calvet, N ; D’Alessio, P ; McClure, M ; Watson, D. M ; Hartmann, L ; Sargent, B</creator><creatorcontrib>Espaillat, C ; Muzerolle, J ; Hernández, J ; Briceño, C ; Calvet, N ; D’Alessio, P ; McClure, M ; Watson, D. M ; Hartmann, L ; Sargent, B</creatorcontrib><description>Here we present the Spitzer IRS spectrum of CVSO 224, the sole transitional disk located within the [image]10 Myr old 25 Orionis group in Orion OB1a. A model fit to the spectral energy distribution of this object indicates a [image]7 AU inner disk hole that contains a small amount of optically thin dust. In previous studies, CVSO 224 had been classified as a weak-line T Tauri star based on its H alpha equivalent width, but here we find an accretion rate of 7 x 10[image] M sub([image]) yr[image] based on high- resolution Hectochelle data. CVSO 224's low [image] is in line with photoevaporative clearing theories. However, the Spitzer IRS spectrum of CVSO 224 has a substantial mid-infrared excess beyond 20 [mu]m which indicates that it is surrounded by a massive outer disk. Millimeter measurements are necessary to constrain the mass of the outer disk around CVSO 224 in order to confirm that photoevaporation is not the mechanism behind creating its inner disk hole.</description><identifier>ISSN: 1538-4357</identifier><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/595869</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Astronomy ; Earth, ocean, space ; Exact sciences and technology</subject><ispartof>The Astrophysical journal, 2008, Vol.689 (2), p.L145-L148</ispartof><rights>2009 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3259-76f23e1a56fa6a00e7d53bc83e31a2fab3b74041021106d96e8c2e8ee17860d43</citedby><cites>FETCH-LOGICAL-c3259-76f23e1a56fa6a00e7d53bc83e31a2fab3b74041021106d96e8c2e8ee17860d43</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1086/595869/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>315,781,785,4025,27633,27928,27929,27930,53936</link.rule.ids><linktorsrc>$$Uhttp://iopscience.iop.org/1538-4357/689/2/L145$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=20956512$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Espaillat, C</creatorcontrib><creatorcontrib>Muzerolle, J</creatorcontrib><creatorcontrib>Hernández, J</creatorcontrib><creatorcontrib>Briceño, C</creatorcontrib><creatorcontrib>Calvet, N</creatorcontrib><creatorcontrib>D’Alessio, P</creatorcontrib><creatorcontrib>McClure, M</creatorcontrib><creatorcontrib>Watson, D. M</creatorcontrib><creatorcontrib>Hartmann, L</creatorcontrib><creatorcontrib>Sargent, B</creatorcontrib><title>A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a</title><title>The Astrophysical journal</title><description>Here we present the Spitzer IRS spectrum of CVSO 224, the sole transitional disk located within the [image]10 Myr old 25 Orionis group in Orion OB1a. A model fit to the spectral energy distribution of this object indicates a [image]7 AU inner disk hole that contains a small amount of optically thin dust. In previous studies, CVSO 224 had been classified as a weak-line T Tauri star based on its H alpha equivalent width, but here we find an accretion rate of 7 x 10[image] M sub([image]) yr[image] based on high- resolution Hectochelle data. CVSO 224's low [image] is in line with photoevaporative clearing theories. However, the Spitzer IRS spectrum of CVSO 224 has a substantial mid-infrared excess beyond 20 [mu]m which indicates that it is surrounded by a massive outer disk. Millimeter measurements are necessary to constrain the mass of the outer disk around CVSO 224 in order to confirm that photoevaporation is not the mechanism behind creating its inner disk hole.</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><issn>1538-4357</issn><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNp90MtKAzEYhuEgCtaq1xAX6kJG8-c0yUao9QiVLqzrkGYyEp3O1KRFuvHandJiFcRVEnj4Ai9Ch0DOgSh5IbRQUm-hDgimMs5Evv3jvov2UnolhHCqdQdd9vBT1XxUC9xzLvpZqF_wJxD8uIhZUxV4FG2dwiw0ta3wdUhvONR4GNs3Hl6B3Uc7pa2SP1ifXfR8ezPq32eD4d1DvzfIHKNCZ7ksKfNghSyttIT4vBBs7BTzDCwt7ZiNc044EApAZKGlV4565T3kSpKCsy46Xe1OY_M-92lmJiE5X1W29s08mZwzLkDmrJUn_0rQHASlcgNdbFKKvjTTGCY2LgwQswxpViFbeLxetMnZqmyLuJC-NSVaSAG0dWcrF5rpZqvtbpbdjVTaUDMALsy0KFt99If-_fMXs0WGAA</recordid><startdate>2008</startdate><enddate>2008</enddate><creator>Espaillat, C</creator><creator>Muzerolle, J</creator><creator>Hernández, J</creator><creator>Briceño, C</creator><creator>Calvet, N</creator><creator>D’Alessio, P</creator><creator>McClure, M</creator><creator>Watson, D. M</creator><creator>Hartmann, L</creator><creator>Sargent, B</creator><general>IOP Publishing</general><general>IOP</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>2008</creationdate><title>A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a</title><author>Espaillat, C ; Muzerolle, J ; Hernández, J ; Briceño, C ; Calvet, N ; D’Alessio, P ; McClure, M ; Watson, D. M ; Hartmann, L ; Sargent, B</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3259-76f23e1a56fa6a00e7d53bc83e31a2fab3b74041021106d96e8c2e8ee17860d43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2008</creationdate><topic>Astronomy</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Espaillat, C</creatorcontrib><creatorcontrib>Muzerolle, J</creatorcontrib><creatorcontrib>Hernández, J</creatorcontrib><creatorcontrib>Briceño, C</creatorcontrib><creatorcontrib>Calvet, N</creatorcontrib><creatorcontrib>D’Alessio, P</creatorcontrib><creatorcontrib>McClure, M</creatorcontrib><creatorcontrib>Watson, D. M</creatorcontrib><creatorcontrib>Hartmann, L</creatorcontrib><creatorcontrib>Sargent, B</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Espaillat, C</au><au>Muzerolle, J</au><au>Hernández, J</au><au>Briceño, C</au><au>Calvet, N</au><au>D’Alessio, P</au><au>McClure, M</au><au>Watson, D. M</au><au>Hartmann, L</au><au>Sargent, B</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a</atitle><jtitle>The Astrophysical journal</jtitle><date>2008</date><risdate>2008</risdate><volume>689</volume><issue>2</issue><spage>L145</spage><epage>L148</epage><pages>L145-L148</pages><issn>1538-4357</issn><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>Here we present the Spitzer IRS spectrum of CVSO 224, the sole transitional disk located within the [image]10 Myr old 25 Orionis group in Orion OB1a. A model fit to the spectral energy distribution of this object indicates a [image]7 AU inner disk hole that contains a small amount of optically thin dust. In previous studies, CVSO 224 had been classified as a weak-line T Tauri star based on its H alpha equivalent width, but here we find an accretion rate of 7 x 10[image] M sub([image]) yr[image] based on high- resolution Hectochelle data. CVSO 224's low [image] is in line with photoevaporative clearing theories. However, the Spitzer IRS spectrum of CVSO 224 has a substantial mid-infrared excess beyond 20 [mu]m which indicates that it is surrounded by a massive outer disk. Millimeter measurements are necessary to constrain the mass of the outer disk around CVSO 224 in order to confirm that photoevaporation is not the mechanism behind creating its inner disk hole.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1086/595869</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 1538-4357 |
ispartof | The Astrophysical journal, 2008, Vol.689 (2), p.L145-L148 |
issn | 1538-4357 0004-637X 1538-4357 |
language | eng |
recordid | cdi_crossref_primary_10_1086_595869 |
source | Institute of Physics Open Access Journal Titles |
subjects | Astronomy Earth, ocean, space Exact sciences and technology |
title | A Slowly Accreting ~10 Myr-old Transitional Disk in Orion OB1a |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-15T20%3A06%3A09IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20Slowly%20Accreting%20~10%20Myr-old%20Transitional%20Disk%20in%20Orion%20OB1a&rft.jtitle=The%20Astrophysical%20journal&rft.au=Espaillat,%20C&rft.date=2008&rft.volume=689&rft.issue=2&rft.spage=L145&rft.epage=L148&rft.pages=L145-L148&rft.issn=1538-4357&rft.eissn=1538-4357&rft.coden=ASJOAB&rft_id=info:doi/10.1086/595869&rft_dat=%3Cproquest_O3W%3E743451673%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=19415226&rft_id=info:pmid/&rfr_iscdi=true |