The First Scattered-light Image of the Debris Disk around the Sco-Cen Target HD 129590
We present the first scattered-light image of the debris disk around HD 129590, a ∼1.3 M G1V member of the Scorpius-Centaurus association with an age of ∼10-16 Myr. The debris disk is imaged with the high contrast imaging instrument SPHERE at the Very Large Telescope, and is revealed by both the IRD...
Gespeichert in:
| Veröffentlicht in: | Astrophysical journal. Letters 2017-07, Vol.843 (1), p.L12 |
|---|---|
| Hauptverfasser: | , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | 1 |
| container_start_page | L12 |
| container_title | Astrophysical journal. Letters |
| container_volume | 843 |
| creator | Matthews, Elisabeth Hinkley, Sasha Vigan, Arthur Kennedy, Grant Rizzuto, Aaron Stapelfeldt, Karl Mawet, Dimitri Booth, Mark Chen, Christine Jang-Condell, Hannah |
| description | We present the first scattered-light image of the debris disk around HD 129590, a ∼1.3 M G1V member of the Scorpius-Centaurus association with an age of ∼10-16 Myr. The debris disk is imaged with the high contrast imaging instrument SPHERE at the Very Large Telescope, and is revealed by both the IRDIS and IFS subsytems, operating in the H and YJ bands respectively. The disk has a high infrared luminosity of ∼ 5 × 10−3, and has been resolved in other studies using ALMA. We detect a nearly edge-on ring, with evidence of an inner clearing. We fit the debris disk using a model characterized by a single bright ring, with radius ∼60-70 au, in broad agreement with previous analyses of the target SED. The disk is vertically thin, and has an inclination angle of ∼75°. Along with other previously imaged edge-on disks in the Sco-Cen association such as HD 110058, HD 115600, and HD 111520, this disk image will allow of the structure and morphology of very young debris disks, shortly after the epoch of planet formation has ceased. |
| doi_str_mv | 10.3847/2041-8213/aa7943 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_crossref_primary_10_3847_2041_8213_aa7943</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365617126</sourcerecordid><originalsourceid>FETCH-LOGICAL-c509t-4fb4be509f196c11051403a4e589270ccd707fbe9431101885a97ab2373e70333</originalsourceid><addsrcrecordid>eNp9kdFLIzEQxhe5A3ue7z4GBOHA1Zlks8k-SqtWKNxDq68hm2bb1LpZk1Twv3frSn057mmGb37zwTeTZWcIV0wW4ppCgbmkyK61FlXBjrLRQfpx6IEfZ79i3ABQKFGOsqfF2pI7F2Iic6NTssEu861brRN5eNErS3xDUo9MbB1cJBMXn4kOftcuP-W58fnYtmShw8omMp0QpBWv4Hf2s9HbaE-_6kn2eHe7GE_z2d_7h_HNLDccqpQXTV3Utm8brEqDCBwLYLqwXFZUgDFLAaKpbZ-nH6KUXFdC15QJZgUwxk6y88HXx-RUNC5Zsza-ba1JilIpaAm8p_4M1FpvVRfciw7vymunpjcztdcASyGZ5G_47dgF_7qzMamN34W2D6EoK3mJAmnZUzBQJvgYg20Otghq_w-1P7jaH18N_-hXLocV57tvz__gF__AdbfZKlkwhWqGVHXLhn0AQieSRg</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365617126</pqid></control><display><type>article</type><title>The First Scattered-light Image of the Debris Disk around the Sco-Cen Target HD 129590</title><source>IOP Publishing Free Content</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>IOPscience extra</source><source>Alma/SFX Local Collection</source><creator>Matthews, Elisabeth ; Hinkley, Sasha ; Vigan, Arthur ; Kennedy, Grant ; Rizzuto, Aaron ; Stapelfeldt, Karl ; Mawet, Dimitri ; Booth, Mark ; Chen, Christine ; Jang-Condell, Hannah</creator><creatorcontrib>Matthews, Elisabeth ; Hinkley, Sasha ; Vigan, Arthur ; Kennedy, Grant ; Rizzuto, Aaron ; Stapelfeldt, Karl ; Mawet, Dimitri ; Booth, Mark ; Chen, Christine ; Jang-Condell, Hannah</creatorcontrib><description>We present the first scattered-light image of the debris disk around HD 129590, a ∼1.3 M G1V member of the Scorpius-Centaurus association with an age of ∼10-16 Myr. The debris disk is imaged with the high contrast imaging instrument SPHERE at the Very Large Telescope, and is revealed by both the IRDIS and IFS subsytems, operating in the H and YJ bands respectively. The disk has a high infrared luminosity of ∼ 5 × 10−3, and has been resolved in other studies using ALMA. We detect a nearly edge-on ring, with evidence of an inner clearing. We fit the debris disk using a model characterized by a single bright ring, with radius ∼60-70 au, in broad agreement with previous analyses of the target SED. The disk is vertically thin, and has an inclination angle of ∼75°. Along with other previously imaged edge-on disks in the Sco-Cen association such as HD 110058, HD 115600, and HD 111520, this disk image will allow of the structure and morphology of very young debris disks, shortly after the epoch of planet formation has ceased.</description><identifier>ISSN: 2041-8205</identifier><identifier>EISSN: 2041-8213</identifier><identifier>DOI: 10.3847/2041-8213/aa7943</identifier><language>eng</language><publisher>Austin: The American Astronomical Society</publisher><subject>Accretion disks ; Astrophysics ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Debris ; Detritus ; INCLINATION ; Inclination angle ; LIGHT SCATTERING ; LUMINOSITY ; MORPHOLOGY ; Planet formation ; planetary systems ; PLANETS ; Sciences of the Universe ; Space telescopes ; STARS ; stars: early-type ; stars: individual (HD 129590) ; TELESCOPES ; Very Large Telescope</subject><ispartof>Astrophysical journal. Letters, 2017-07, Vol.843 (1), p.L12</ispartof><rights>2017. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Jul 01, 2017</rights><rights>Attribution</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c509t-4fb4be509f196c11051403a4e589270ccd707fbe9431101885a97ab2373e70333</citedby><cites>FETCH-LOGICAL-c509t-4fb4be509f196c11051403a4e589270ccd707fbe9431101885a97ab2373e70333</cites><orcidid>0000-0002-7639-1322 ; 0000-0001-8074-2562 ; 0000-0001-6831-7547 ; 0000-0002-8895-4735 ; 0000-0002-8382-0447 ; 0000-0001-9982-1332 ; 0000-0003-0593-1560 ; 0000-0002-5902-7828 ; 0000-0002-2805-7338</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8213/aa7943/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>230,314,776,780,881,27901,27902,38845,38867,53815,53842</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01678385$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/22872605$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Matthews, Elisabeth</creatorcontrib><creatorcontrib>Hinkley, Sasha</creatorcontrib><creatorcontrib>Vigan, Arthur</creatorcontrib><creatorcontrib>Kennedy, Grant</creatorcontrib><creatorcontrib>Rizzuto, Aaron</creatorcontrib><creatorcontrib>Stapelfeldt, Karl</creatorcontrib><creatorcontrib>Mawet, Dimitri</creatorcontrib><creatorcontrib>Booth, Mark</creatorcontrib><creatorcontrib>Chen, Christine</creatorcontrib><creatorcontrib>Jang-Condell, Hannah</creatorcontrib><title>The First Scattered-light Image of the Debris Disk around the Sco-Cen Target HD 129590</title><title>Astrophysical journal. Letters</title><addtitle>APJL</addtitle><addtitle>Astrophys. J. Lett</addtitle><description>We present the first scattered-light image of the debris disk around HD 129590, a ∼1.3 M G1V member of the Scorpius-Centaurus association with an age of ∼10-16 Myr. The debris disk is imaged with the high contrast imaging instrument SPHERE at the Very Large Telescope, and is revealed by both the IRDIS and IFS subsytems, operating in the H and YJ bands respectively. The disk has a high infrared luminosity of ∼ 5 × 10−3, and has been resolved in other studies using ALMA. We detect a nearly edge-on ring, with evidence of an inner clearing. We fit the debris disk using a model characterized by a single bright ring, with radius ∼60-70 au, in broad agreement with previous analyses of the target SED. The disk is vertically thin, and has an inclination angle of ∼75°. Along with other previously imaged edge-on disks in the Sco-Cen association such as HD 110058, HD 115600, and HD 111520, this disk image will allow of the structure and morphology of very young debris disks, shortly after the epoch of planet formation has ceased.</description><subject>Accretion disks</subject><subject>Astrophysics</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Debris</subject><subject>Detritus</subject><subject>INCLINATION</subject><subject>Inclination angle</subject><subject>LIGHT SCATTERING</subject><subject>LUMINOSITY</subject><subject>MORPHOLOGY</subject><subject>Planet formation</subject><subject>planetary systems</subject><subject>PLANETS</subject><subject>Sciences of the Universe</subject><subject>Space telescopes</subject><subject>STARS</subject><subject>stars: early-type</subject><subject>stars: individual (HD 129590)</subject><subject>TELESCOPES</subject><subject>Very Large Telescope</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><recordid>eNp9kdFLIzEQxhe5A3ue7z4GBOHA1Zlks8k-SqtWKNxDq68hm2bb1LpZk1Twv3frSn057mmGb37zwTeTZWcIV0wW4ppCgbmkyK61FlXBjrLRQfpx6IEfZ79i3ABQKFGOsqfF2pI7F2Iic6NTssEu861brRN5eNErS3xDUo9MbB1cJBMXn4kOftcuP-W58fnYtmShw8omMp0QpBWv4Hf2s9HbaE-_6kn2eHe7GE_z2d_7h_HNLDccqpQXTV3Utm8brEqDCBwLYLqwXFZUgDFLAaKpbZ-nH6KUXFdC15QJZgUwxk6y88HXx-RUNC5Zsza-ba1JilIpaAm8p_4M1FpvVRfciw7vymunpjcztdcASyGZ5G_47dgF_7qzMamN34W2D6EoK3mJAmnZUzBQJvgYg20Otghq_w-1P7jaH18N_-hXLocV57tvz__gF__AdbfZKlkwhWqGVHXLhn0AQieSRg</recordid><startdate>20170701</startdate><enddate>20170701</enddate><creator>Matthews, Elisabeth</creator><creator>Hinkley, Sasha</creator><creator>Vigan, Arthur</creator><creator>Kennedy, Grant</creator><creator>Rizzuto, Aaron</creator><creator>Stapelfeldt, Karl</creator><creator>Mawet, Dimitri</creator><creator>Booth, Mark</creator><creator>Chen, Christine</creator><creator>Jang-Condell, Hannah</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><general>Bristol : 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><scope>1XC</scope><scope>VOOES</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-7639-1322</orcidid><orcidid>https://orcid.org/0000-0001-8074-2562</orcidid><orcidid>https://orcid.org/0000-0001-6831-7547</orcidid><orcidid>https://orcid.org/0000-0002-8895-4735</orcidid><orcidid>https://orcid.org/0000-0002-8382-0447</orcidid><orcidid>https://orcid.org/0000-0001-9982-1332</orcidid><orcidid>https://orcid.org/0000-0003-0593-1560</orcidid><orcidid>https://orcid.org/0000-0002-5902-7828</orcidid><orcidid>https://orcid.org/0000-0002-2805-7338</orcidid></search><sort><creationdate>20170701</creationdate><title>The First Scattered-light Image of the Debris Disk around the Sco-Cen Target HD 129590</title><author>Matthews, Elisabeth ; Hinkley, Sasha ; Vigan, Arthur ; Kennedy, Grant ; Rizzuto, Aaron ; Stapelfeldt, Karl ; Mawet, Dimitri ; Booth, Mark ; Chen, Christine ; Jang-Condell, Hannah</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c509t-4fb4be509f196c11051403a4e589270ccd707fbe9431101885a97ab2373e70333</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Accretion disks</topic><topic>Astrophysics</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Debris</topic><topic>Detritus</topic><topic>INCLINATION</topic><topic>Inclination angle</topic><topic>LIGHT SCATTERING</topic><topic>LUMINOSITY</topic><topic>MORPHOLOGY</topic><topic>Planet formation</topic><topic>planetary systems</topic><topic>PLANETS</topic><topic>Sciences of the Universe</topic><topic>Space telescopes</topic><topic>STARS</topic><topic>stars: early-type</topic><topic>stars: individual (HD 129590)</topic><topic>TELESCOPES</topic><topic>Very Large Telescope</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Matthews, Elisabeth</creatorcontrib><creatorcontrib>Hinkley, Sasha</creatorcontrib><creatorcontrib>Vigan, Arthur</creatorcontrib><creatorcontrib>Kennedy, Grant</creatorcontrib><creatorcontrib>Rizzuto, Aaron</creatorcontrib><creatorcontrib>Stapelfeldt, Karl</creatorcontrib><creatorcontrib>Mawet, Dimitri</creatorcontrib><creatorcontrib>Booth, Mark</creatorcontrib><creatorcontrib>Chen, Christine</creatorcontrib><creatorcontrib>Jang-Condell, Hannah</creatorcontrib><collection>IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><collection>OSTI.GOV</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Matthews, Elisabeth</au><au>Hinkley, Sasha</au><au>Vigan, Arthur</au><au>Kennedy, Grant</au><au>Rizzuto, Aaron</au><au>Stapelfeldt, Karl</au><au>Mawet, Dimitri</au><au>Booth, Mark</au><au>Chen, Christine</au><au>Jang-Condell, Hannah</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The First Scattered-light Image of the Debris Disk around the Sco-Cen Target HD 129590</atitle><jtitle>Astrophysical journal. Letters</jtitle><stitle>APJL</stitle><addtitle>Astrophys. J. Lett</addtitle><date>2017-07-01</date><risdate>2017</risdate><volume>843</volume><issue>1</issue><spage>L12</spage><pages>L12-</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>We present the first scattered-light image of the debris disk around HD 129590, a ∼1.3 M G1V member of the Scorpius-Centaurus association with an age of ∼10-16 Myr. The debris disk is imaged with the high contrast imaging instrument SPHERE at the Very Large Telescope, and is revealed by both the IRDIS and IFS subsytems, operating in the H and YJ bands respectively. The disk has a high infrared luminosity of ∼ 5 × 10−3, and has been resolved in other studies using ALMA. We detect a nearly edge-on ring, with evidence of an inner clearing. We fit the debris disk using a model characterized by a single bright ring, with radius ∼60-70 au, in broad agreement with previous analyses of the target SED. The disk is vertically thin, and has an inclination angle of ∼75°. Along with other previously imaged edge-on disks in the Sco-Cen association such as HD 110058, HD 115600, and HD 111520, this disk image will allow of the structure and morphology of very young debris disks, shortly after the epoch of planet formation has ceased.</abstract><cop>Austin</cop><pub>The American Astronomical Society</pub><doi>10.3847/2041-8213/aa7943</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0002-7639-1322</orcidid><orcidid>https://orcid.org/0000-0001-8074-2562</orcidid><orcidid>https://orcid.org/0000-0001-6831-7547</orcidid><orcidid>https://orcid.org/0000-0002-8895-4735</orcidid><orcidid>https://orcid.org/0000-0002-8382-0447</orcidid><orcidid>https://orcid.org/0000-0001-9982-1332</orcidid><orcidid>https://orcid.org/0000-0003-0593-1560</orcidid><orcidid>https://orcid.org/0000-0002-5902-7828</orcidid><orcidid>https://orcid.org/0000-0002-2805-7338</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 2041-8205 |
| ispartof | Astrophysical journal. Letters, 2017-07, Vol.843 (1), p.L12 |
| issn | 2041-8205 2041-8213 |
| language | eng |
| recordid | cdi_crossref_primary_10_3847_2041_8213_aa7943 |
| source | IOP Publishing Free Content; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; IOPscience extra; Alma/SFX Local Collection |
| subjects | Accretion disks Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Debris Detritus INCLINATION Inclination angle LIGHT SCATTERING LUMINOSITY MORPHOLOGY Planet formation planetary systems PLANETS Sciences of the Universe Space telescopes STARS stars: early-type stars: individual (HD 129590) TELESCOPES Very Large Telescope |
| title | The First Scattered-light Image of the Debris Disk around the Sco-Cen Target HD 129590 |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-20T16%3A30%3A27IST&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=The%20First%20Scattered-light%20Image%20of%20the%20Debris%20Disk%20around%20the%20Sco-Cen%20Target%20HD%20129590&rft.jtitle=Astrophysical%20journal.%20Letters&rft.au=Matthews,%20Elisabeth&rft.date=2017-07-01&rft.volume=843&rft.issue=1&rft.spage=L12&rft.pages=L12-&rft.issn=2041-8205&rft.eissn=2041-8213&rft_id=info:doi/10.3847/2041-8213/aa7943&rft_dat=%3Cproquest_cross%3E2365617126%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=2365617126&rft_id=info:pmid/&rfr_iscdi=true |