Disk of 2MASS 15491331−3539118 = GQ Lup C as seen by HST and WISE
Aims. Very recently, a second companion on a wider orbit has been discovered around GQ Lup. This is a low-mass accreting star that is partially obscured by a disk seen at high inclination. If detected, this disk may be compared to the known disk around the primary. Methods. We detected this disk on...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2020-03, Vol.635, p.L11 |
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container_title | Astronomy and astrophysics (Berlin) |
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creator | Lazzoni, C. Gratton, R. Alcalá, J. M. Desidera, S. Frasca, A. Manara, C. F. Mesa, D. Rigliaco, E. Vigan, A. Zurlo, A. |
description | Aims.
Very recently, a second companion on a wider orbit has been discovered around GQ Lup. This is a low-mass accreting star that is partially obscured by a disk seen at high inclination. If detected, this disk may be compared to the known disk around the primary.
Methods.
We detected this disk on archive HST and WISE data.
Results.
The extended spectral energy distribution provided by these data confirms the presence of accretion from H
α
emission and UV excess, and shows an IR excess attributable to a warm disk. In addition, we resolved the disk on the HST images. It is found to be roughly aligned with the disk of the primary. Both of them are roughly aligned with the Lupus I dust filament containing GQ Lup. |
doi_str_mv | 10.1051/0004-6361/202037622 |
format | Article |
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Very recently, a second companion on a wider orbit has been discovered around GQ Lup. This is a low-mass accreting star that is partially obscured by a disk seen at high inclination. If detected, this disk may be compared to the known disk around the primary.
Methods.
We detected this disk on archive HST and WISE data.
Results.
The extended spectral energy distribution provided by these data confirms the presence of accretion from H
α
emission and UV excess, and shows an IR excess attributable to a warm disk. In addition, we resolved the disk on the HST images. It is found to be roughly aligned with the disk of the primary. Both of them are roughly aligned with the Lupus I dust filament containing GQ Lup.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>EISSN: 1432-0756</identifier><identifier>DOI: 10.1051/0004-6361/202037622</identifier><language>eng</language><publisher>Heidelberg: EDP Sciences</publisher><subject>Astrophysics ; Sciences of the Universe</subject><ispartof>Astronomy and astrophysics (Berlin), 2020-03, Vol.635, p.L11</ispartof><rights>Copyright EDP Sciences Mar 2020</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c356t-914e238cae82eb115319d4794cdc2a30cd824d98dd345075814f990ff04374af3</citedby><cites>FETCH-LOGICAL-c356t-914e238cae82eb115319d4794cdc2a30cd824d98dd345075814f990ff04374af3</cites><orcidid>0000-0001-7819-9003 ; 0000-0001-8467-1933 ; 0000-0003-2195-6805 ; 0000-0002-0474-0896 ; 0000-0003-1401-6444 ; 0000-0002-5903-8316 ; 0000-0003-3562-262X ; 0000-0001-8613-2589 ; 0000-0002-5902-7828 ; 0000-0001-8657-095X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,3714,27901,27902</link.rule.ids><backlink>$$Uhttps://hal.science/hal-02899002$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Lazzoni, C.</creatorcontrib><creatorcontrib>Gratton, R.</creatorcontrib><creatorcontrib>Alcalá, J. M.</creatorcontrib><creatorcontrib>Desidera, S.</creatorcontrib><creatorcontrib>Frasca, A.</creatorcontrib><creatorcontrib>Manara, C. F.</creatorcontrib><creatorcontrib>Mesa, D.</creatorcontrib><creatorcontrib>Rigliaco, E.</creatorcontrib><creatorcontrib>Vigan, A.</creatorcontrib><creatorcontrib>Zurlo, A.</creatorcontrib><title>Disk of 2MASS 15491331−3539118 = GQ Lup C as seen by HST and WISE</title><title>Astronomy and astrophysics (Berlin)</title><description>Aims.
Very recently, a second companion on a wider orbit has been discovered around GQ Lup. This is a low-mass accreting star that is partially obscured by a disk seen at high inclination. If detected, this disk may be compared to the known disk around the primary.
Methods.
We detected this disk on archive HST and WISE data.
Results.
The extended spectral energy distribution provided by these data confirms the presence of accretion from H
α
emission and UV excess, and shows an IR excess attributable to a warm disk. In addition, we resolved the disk on the HST images. It is found to be roughly aligned with the disk of the primary. Both of them are roughly aligned with the Lupus I dust filament containing GQ Lup.</description><subject>Astrophysics</subject><subject>Sciences of the Universe</subject><issn>0004-6361</issn><issn>1432-0746</issn><issn>1432-0756</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNo9kMFKw0AQhhdRsFafwMuCJw-xOzuzye7BQ4m1LUREUvG4bJMNtmpTs63QN_DsI_okJlR6Gmb4_p_hY-wSxA0IBQMhBEUxxjCQQgpMYimPWA8IZSQSio9Z70CcsrMQlu0qQWOPpXeL8MbrisuHYZ5zUGQAEX6_f1ChAdD8lo-feLZd85S7wIP3Kz7f8Uk-425V8pdpPjpnJ5V7D_7if_bZ8_1olk6i7HE8TYdZVKCKN5EB8hJ14byWfg6gEExJiaGiLKRDUZRaUml0WSIpkSgNVBkjqkoQJuQq7LPrfe-re7frZvHhmp2t3cJOhpntbkLqNiDkF7Ts1Z5dN_Xn1oeNXdbbZtW-ZyXpBIAoxpbCPVU0dQiNrw61IGxn1nbebOfNHsziH_F7YxM</recordid><startdate>20200301</startdate><enddate>20200301</enddate><creator>Lazzoni, C.</creator><creator>Gratton, R.</creator><creator>Alcalá, J. M.</creator><creator>Desidera, S.</creator><creator>Frasca, A.</creator><creator>Manara, C. F.</creator><creator>Mesa, D.</creator><creator>Rigliaco, E.</creator><creator>Vigan, A.</creator><creator>Zurlo, A.</creator><general>EDP Sciences</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>1XC</scope><scope>VOOES</scope><orcidid>https://orcid.org/0000-0001-7819-9003</orcidid><orcidid>https://orcid.org/0000-0001-8467-1933</orcidid><orcidid>https://orcid.org/0000-0003-2195-6805</orcidid><orcidid>https://orcid.org/0000-0002-0474-0896</orcidid><orcidid>https://orcid.org/0000-0003-1401-6444</orcidid><orcidid>https://orcid.org/0000-0002-5903-8316</orcidid><orcidid>https://orcid.org/0000-0003-3562-262X</orcidid><orcidid>https://orcid.org/0000-0001-8613-2589</orcidid><orcidid>https://orcid.org/0000-0002-5902-7828</orcidid><orcidid>https://orcid.org/0000-0001-8657-095X</orcidid></search><sort><creationdate>20200301</creationdate><title>Disk of 2MASS 15491331−3539118 = GQ Lup C as seen by HST and WISE</title><author>Lazzoni, C. ; Gratton, R. ; Alcalá, J. M. ; Desidera, S. ; Frasca, A. ; Manara, C. F. ; Mesa, D. ; Rigliaco, E. ; Vigan, A. ; Zurlo, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c356t-914e238cae82eb115319d4794cdc2a30cd824d98dd345075814f990ff04374af3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Astrophysics</topic><topic>Sciences of the Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Lazzoni, C.</creatorcontrib><creatorcontrib>Gratton, R.</creatorcontrib><creatorcontrib>Alcalá, J. M.</creatorcontrib><creatorcontrib>Desidera, S.</creatorcontrib><creatorcontrib>Frasca, A.</creatorcontrib><creatorcontrib>Manara, C. F.</creatorcontrib><creatorcontrib>Mesa, D.</creatorcontrib><creatorcontrib>Rigliaco, E.</creatorcontrib><creatorcontrib>Vigan, A.</creatorcontrib><creatorcontrib>Zurlo, A.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lazzoni, C.</au><au>Gratton, R.</au><au>Alcalá, J. M.</au><au>Desidera, S.</au><au>Frasca, A.</au><au>Manara, C. F.</au><au>Mesa, D.</au><au>Rigliaco, E.</au><au>Vigan, A.</au><au>Zurlo, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Disk of 2MASS 15491331−3539118 = GQ Lup C as seen by HST and WISE</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2020-03-01</date><risdate>2020</risdate><volume>635</volume><spage>L11</spage><pages>L11-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><eissn>1432-0756</eissn><abstract>Aims.
Very recently, a second companion on a wider orbit has been discovered around GQ Lup. This is a low-mass accreting star that is partially obscured by a disk seen at high inclination. If detected, this disk may be compared to the known disk around the primary.
Methods.
We detected this disk on archive HST and WISE data.
Results.
The extended spectral energy distribution provided by these data confirms the presence of accretion from H
α
emission and UV excess, and shows an IR excess attributable to a warm disk. In addition, we resolved the disk on the HST images. It is found to be roughly aligned with the disk of the primary. Both of them are roughly aligned with the Lupus I dust filament containing GQ Lup.</abstract><cop>Heidelberg</cop><pub>EDP Sciences</pub><doi>10.1051/0004-6361/202037622</doi><orcidid>https://orcid.org/0000-0001-7819-9003</orcidid><orcidid>https://orcid.org/0000-0001-8467-1933</orcidid><orcidid>https://orcid.org/0000-0003-2195-6805</orcidid><orcidid>https://orcid.org/0000-0002-0474-0896</orcidid><orcidid>https://orcid.org/0000-0003-1401-6444</orcidid><orcidid>https://orcid.org/0000-0002-5903-8316</orcidid><orcidid>https://orcid.org/0000-0003-3562-262X</orcidid><orcidid>https://orcid.org/0000-0001-8613-2589</orcidid><orcidid>https://orcid.org/0000-0002-5902-7828</orcidid><orcidid>https://orcid.org/0000-0001-8657-095X</orcidid><oa>free_for_read</oa></addata></record> |
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source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
subjects | Astrophysics Sciences of the Universe |
title | Disk of 2MASS 15491331−3539118 = GQ Lup C as seen by HST and WISE |
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