Strong Near-Infrared Emission Interior to the Dust Sublimation Radius of Young Stellar Objects MWC 275 and AB Aurigae

Strong Near-Infrared Emission Interior to the Dust Sublimation Radius of Young Stellar Objects MWC 275 and AB Aurigae

Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust destruction radius of Herbig Ae stars MWC 275 and AB Aur. Our submilliarcsecond resolution observations unambiguously place the emission between the dus...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2008-04, Vol.677 (1), p.L51-L54
Hauptverfasser: Tannirkulam, A, Monnier, J. D, Millan-Gabet, R, Harries, T. J, Pedretti, E, ten Brummelaar, T. A, McAlister, H, Turner, N, Sturmann, J, Sturmann, L
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Earth, ocean, space
Exact sciences and technology
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page L54
container_issue 1
container_start_page L51
container_title The Astrophysical journal
container_volume 677
creator Tannirkulam, A
Monnier, J. D
Millan-Gabet, R
Harries, T. J
Pedretti, E
ten Brummelaar, T. A
McAlister, H
Turner, N
Sturmann, J
Sturmann, L
description Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust destruction radius of Herbig Ae stars MWC 275 and AB Aur. Our submilliarcsecond resolution observations unambiguously place the emission between the dust destruction radius and the magnetospheric corotation radius. We argue that this new component corresponds to hot gas inside the dust sublimation radius, confirming recent claims based on spectrally resolved interferometry and dust evaporation front modeling.
doi_str_mv 10.1086/587873
format Article
fullrecord <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_iop_primary_10_1086_587873</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>20911541</sourcerecordid><originalsourceid>FETCH-LOGICAL-c475t-106bf227fc788a7bad71a2da1896ec31c0bd70023e5826b09029b74da3d08f643</originalsourceid><addsrcrecordid>eNp90U9LwzAYBvAiCs6pnyEeVBCq-dukxzmnDqYDp4inkCbp7KjNTNKD396ODfWgnt4cfjzkfd4kOUTwHEGRXTDBBSdbSQ8xIlJKGN_-8d5N9kJYQAgpzvNe0s6id80c3Fvl03FTeuWtAaO3KoTKNWDcROsr50F0IL5acNWGCGZtUVdvKq7AgzJVG4ArwYtru5xZtHWtPJgWC6tjAHfPQ4A5A6oxYHAJBq2v5sruJzulqoM92Mx-8nQ9ehzeppPpzXg4mKSachZTBLOixJiXmguheKEMRwobhUSeWU2QhoXhEGJimcBZAXOI84JTo4iBoswo6Sen69yld--tDVF2i-nVDxvr2iA5JVQwnONOnvwrMcwRYhR9Q-1dCN6Wcum7MvyHRFCu-pfr_jt4vElUQau6a7bRVfjSGGKOCOWdO1q7yi3_zjr7xXQnlauTyoxzieSEIbk0JfkE8fGZ8Q</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>20911541</pqid></control><display><type>article</type><title>Strong Near-Infrared Emission Interior to the Dust Sublimation Radius of Young Stellar Objects MWC 275 and AB Aurigae</title><source>IOP Publishing</source><creator>Tannirkulam, A ; Monnier, J. D ; Millan-Gabet, R ; Harries, T. J ; Pedretti, E ; ten Brummelaar, T. A ; McAlister, H ; Turner, N ; Sturmann, J ; Sturmann, L</creator><creatorcontrib>Tannirkulam, A ; Monnier, J. D ; Millan-Gabet, R ; Harries, T. J ; Pedretti, E ; ten Brummelaar, T. A ; McAlister, H ; Turner, N ; Sturmann, J ; Sturmann, L</creatorcontrib><description>Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust destruction radius of Herbig Ae stars MWC 275 and AB Aur. Our submilliarcsecond resolution observations unambiguously place the emission between the dust destruction radius and the magnetospheric corotation radius. We argue that this new component corresponds to hot gas inside the dust sublimation radius, confirming recent claims based on spectrally resolved interferometry and dust evaporation front modeling.</description><identifier>ISSN: 1538-4357</identifier><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/587873</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Chicago, IL: IOP Publishing</publisher><subject>Astronomy ; Earth, ocean, space ; Exact sciences and technology</subject><ispartof>The Astrophysical journal, 2008-04, Vol.677 (1), p.L51-L54</ispartof><rights>2008 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c475t-106bf227fc788a7bad71a2da1896ec31c0bd70023e5826b09029b74da3d08f643</citedby><cites>FETCH-LOGICAL-c475t-106bf227fc788a7bad71a2da1896ec31c0bd70023e5826b09029b74da3d08f643</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1086/587873/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,776,780,27605,27901,27902,53906</link.rule.ids><linktorsrc>$$Uhttp://iopscience.iop.org/1538-4357/677/1/L51$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=20271347$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Tannirkulam, A</creatorcontrib><creatorcontrib>Monnier, J. D</creatorcontrib><creatorcontrib>Millan-Gabet, R</creatorcontrib><creatorcontrib>Harries, T. J</creatorcontrib><creatorcontrib>Pedretti, E</creatorcontrib><creatorcontrib>ten Brummelaar, T. A</creatorcontrib><creatorcontrib>McAlister, H</creatorcontrib><creatorcontrib>Turner, N</creatorcontrib><creatorcontrib>Sturmann, J</creatorcontrib><creatorcontrib>Sturmann, L</creatorcontrib><title>Strong Near-Infrared Emission Interior to the Dust Sublimation Radius of Young Stellar Objects MWC 275 and AB Aurigae</title><title>The Astrophysical journal</title><description>Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust destruction radius of Herbig Ae stars MWC 275 and AB Aur. Our submilliarcsecond resolution observations unambiguously place the emission between the dust destruction radius and the magnetospheric corotation radius. We argue that this new component corresponds to hot gas inside the dust sublimation radius, confirming recent claims based on spectrally resolved interferometry and dust evaporation front modeling.</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>eNp90U9LwzAYBvAiCs6pnyEeVBCq-dukxzmnDqYDp4inkCbp7KjNTNKD396ODfWgnt4cfjzkfd4kOUTwHEGRXTDBBSdbSQ8xIlJKGN_-8d5N9kJYQAgpzvNe0s6id80c3Fvl03FTeuWtAaO3KoTKNWDcROsr50F0IL5acNWGCGZtUVdvKq7AgzJVG4ArwYtru5xZtHWtPJgWC6tjAHfPQ4A5A6oxYHAJBq2v5sruJzulqoM92Mx-8nQ9ehzeppPpzXg4mKSachZTBLOixJiXmguheKEMRwobhUSeWU2QhoXhEGJimcBZAXOI84JTo4iBoswo6Sen69yld--tDVF2i-nVDxvr2iA5JVQwnONOnvwrMcwRYhR9Q-1dCN6Wcum7MvyHRFCu-pfr_jt4vElUQau6a7bRVfjSGGKOCOWdO1q7yi3_zjr7xXQnlauTyoxzieSEIbk0JfkE8fGZ8Q</recordid><startdate>20080410</startdate><enddate>20080410</enddate><creator>Tannirkulam, A</creator><creator>Monnier, J. D</creator><creator>Millan-Gabet, R</creator><creator>Harries, T. J</creator><creator>Pedretti, E</creator><creator>ten Brummelaar, T. A</creator><creator>McAlister, H</creator><creator>Turner, N</creator><creator>Sturmann, J</creator><creator>Sturmann, L</creator><general>IOP Publishing</general><general>University of Chicago Press</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>20080410</creationdate><title>Strong Near-Infrared Emission Interior to the Dust Sublimation Radius of Young Stellar Objects MWC 275 and AB Aurigae</title><author>Tannirkulam, A ; Monnier, J. D ; Millan-Gabet, R ; Harries, T. J ; Pedretti, E ; ten Brummelaar, T. A ; McAlister, H ; Turner, N ; Sturmann, J ; Sturmann, L</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c475t-106bf227fc788a7bad71a2da1896ec31c0bd70023e5826b09029b74da3d08f643</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>Tannirkulam, A</creatorcontrib><creatorcontrib>Monnier, J. D</creatorcontrib><creatorcontrib>Millan-Gabet, R</creatorcontrib><creatorcontrib>Harries, T. J</creatorcontrib><creatorcontrib>Pedretti, E</creatorcontrib><creatorcontrib>ten Brummelaar, T. A</creatorcontrib><creatorcontrib>McAlister, H</creatorcontrib><creatorcontrib>Turner, N</creatorcontrib><creatorcontrib>Sturmann, J</creatorcontrib><creatorcontrib>Sturmann, L</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; 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>Tannirkulam, A</au><au>Monnier, J. D</au><au>Millan-Gabet, R</au><au>Harries, T. J</au><au>Pedretti, E</au><au>ten Brummelaar, T. A</au><au>McAlister, H</au><au>Turner, N</au><au>Sturmann, J</au><au>Sturmann, L</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Strong Near-Infrared Emission Interior to the Dust Sublimation Radius of Young Stellar Objects MWC 275 and AB Aurigae</atitle><jtitle>The Astrophysical journal</jtitle><date>2008-04-10</date><risdate>2008</risdate><volume>677</volume><issue>1</issue><spage>L51</spage><epage>L54</epage><pages>L51-L54</pages><issn>1538-4357</issn><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust destruction radius of Herbig Ae stars MWC 275 and AB Aur. Our submilliarcsecond resolution observations unambiguously place the emission between the dust destruction radius and the magnetospheric corotation radius. We argue that this new component corresponds to hot gas inside the dust sublimation radius, confirming recent claims based on spectrally resolved interferometry and dust evaporation front modeling.</abstract><cop>Chicago, IL</cop><pub>IOP Publishing</pub><doi>10.1086/587873</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 1538-4357
ispartof The Astrophysical journal, 2008-04, Vol.677 (1), p.L51-L54
issn 1538-4357
0004-637X
1538-4357
language eng
recordid cdi_iop_primary_10_1086_587873
source IOP Publishing
subjects Astronomy
Earth, ocean, space
Exact sciences and technology
title Strong Near-Infrared Emission Interior to the Dust Sublimation Radius of Young Stellar Objects MWC 275 and AB Aurigae
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-12T00%3A51%3A38IST&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=Strong%20Near-Infrared%20Emission%20Interior%20to%20the%20Dust%20Sublimation%20Radius%20of%20Young%20Stellar%20Objects%20MWC%20275%20and%20AB%20Aurigae&rft.jtitle=The%20Astrophysical%20journal&rft.au=Tannirkulam,%20A&rft.date=2008-04-10&rft.volume=677&rft.issue=1&rft.spage=L51&rft.epage=L54&rft.pages=L51-L54&rft.issn=1538-4357&rft.eissn=1538-4357&rft.coden=ASJOAB&rft_id=info:doi/10.1086/587873&rft_dat=%3Cproquest_O3W%3E20911541%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=20911541&rft_id=info:pmid/&rfr_iscdi=true