A DWARF TRANSITIONAL PROTOPLANETARY DISK AROUND XZ TAU B

ABSTRACT We report the discovery of a dwarf protoplanetary disk around the star XZ Tau B that shows all the features of a classical transitional disk but on a much smaller scale. The disk has been imaged with the Atacama Large Millimeter/submillimeter Array (ALMA), revealing that its dust emission h...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astrophysical journal. Letters 2016-07, Vol.825 (1), p.L10-L10
Hauptverfasser: Osorio, Mayra, Macías, Enrique, Anglada, Guillem, Carrasco-González, Carlos, Galván-Madrid, Roberto, Zapata, Luis, Calvet, Nuria, Gómez, José F., Nagel, Erick, Rodríguez, Luis F., Torrelles, José M., Zhu, Zhaohuan
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page L10
container_issue 1
container_start_page L10
container_title Astrophysical journal. Letters
container_volume 825
creator Osorio, Mayra
Macías, Enrique
Anglada, Guillem
Carrasco-González, Carlos
Galván-Madrid, Roberto
Zapata, Luis
Calvet, Nuria
Gómez, José F.
Nagel, Erick
Rodríguez, Luis F.
Torrelles, José M.
Zhu, Zhaohuan
description ABSTRACT We report the discovery of a dwarf protoplanetary disk around the star XZ Tau B that shows all the features of a classical transitional disk but on a much smaller scale. The disk has been imaged with the Atacama Large Millimeter/submillimeter Array (ALMA), revealing that its dust emission has a quite small radius of ∼3.4 au and presents a central cavity of ∼1.3 au in radius that we attribute to clearing by a compact system of orbiting (proto)planets. Given the very small radii involved, evolution is expected to be much faster in this disk (observable changes in a few months) than in classical disks (observable changes requiring decades) and easy to monitor with observations in the near future. From our modeling we estimate that the mass of the disk is large enough to form a compact planetary system.
doi_str_mv 10.3847/2041-8205/825/1/L10
format Article
fullrecord <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_miscellaneous_1884130128</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1884130128</sourcerecordid><originalsourceid>FETCH-LOGICAL-c525t-1d13749ebde4311fda705798c97cdf543632a424647b901d1e214f60e0ecefb63</originalsourceid><addsrcrecordid>eNqNkMtOg0AUQInRxFr9AjckJsYNMk8YlqNtlUigoTQ-NhM6DJGGAjJ04d8LodGNiW7mTm7OuYtjGJcQ3GJGXBsBAi2GALUZoja0AwiOjMlhC_Hx9x_QU-NM6y0ACDiQTQzGzdkzjxdmEvNw5Sd-FPLAXMZREi0DHs4THr-aM3_1ZPI4Wocz8-XNTPjavDs3TvK01OriMKfGejFP7h-tIHrw73lgSYpoZ8EMYpd4apMpgiHMs9QF1PWY9FyZ5ZRgB6OUIOIQd-OBnlYIktwBCiip8o2Dp8bVeLfWXSG0LDol32VdVUp2AiGHEuSBnroZqaatP_ZKd2JXaKnKMq1UvdcCMkYgBhCxf6Cu24dyyIDiEZVtrXWrctG0xS5tPwUEYggvhqxiyNo_VEDRh-8te7SKuhHbet9WfZ8_jOtfjLTZlj-QaLIcfwF5HYlS</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1877820648</pqid></control><display><type>article</type><title>A DWARF TRANSITIONAL PROTOPLANETARY DISK AROUND XZ TAU B</title><source>IOP Publishing Free Content</source><creator>Osorio, Mayra ; Macías, Enrique ; Anglada, Guillem ; Carrasco-González, Carlos ; Galván-Madrid, Roberto ; Zapata, Luis ; Calvet, Nuria ; Gómez, José F. ; Nagel, Erick ; Rodríguez, Luis F. ; Torrelles, José M. ; Zhu, Zhaohuan</creator><creatorcontrib>Osorio, Mayra ; Macías, Enrique ; Anglada, Guillem ; Carrasco-González, Carlos ; Galván-Madrid, Roberto ; Zapata, Luis ; Calvet, Nuria ; Gómez, José F. ; Nagel, Erick ; Rodríguez, Luis F. ; Torrelles, José M. ; Zhu, Zhaohuan</creatorcontrib><description>ABSTRACT We report the discovery of a dwarf protoplanetary disk around the star XZ Tau B that shows all the features of a classical transitional disk but on a much smaller scale. The disk has been imaged with the Atacama Large Millimeter/submillimeter Array (ALMA), revealing that its dust emission has a quite small radius of ∼3.4 au and presents a central cavity of ∼1.3 au in radius that we attribute to clearing by a compact system of orbiting (proto)planets. Given the very small radii involved, evolution is expected to be much faster in this disk (observable changes in a few months) than in classical disks (observable changes requiring decades) and easy to monitor with observations in the near future. From our modeling we estimate that the mass of the disk is large enough to form a compact planetary system.</description><identifier>ISSN: 2041-8205</identifier><identifier>EISSN: 2041-8213</identifier><identifier>DOI: 10.3847/2041-8205/825/1/L10</identifier><language>eng</language><publisher>United States: The American Astronomical Society</publisher><subject>Arrays ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; DUSTS ; DWARF STARS ; EMISSION ; EVOLUTION ; Holes ; INTERACTIONS ; MASS ; MONITORS ; Planet formation ; planet-disk interactions ; PLANETS ; protoplanetary disks ; PROTOPLANETS ; Radio telescopes ; SIMULATION ; STARS ; stars: formation ; stars: individual (XZ Tau B) ; stars: pre-main sequence</subject><ispartof>Astrophysical journal. Letters, 2016-07, Vol.825 (1), p.L10-L10</ispartof><rights>2016. The American Astronomical Society. All rights reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c525t-1d13749ebde4311fda705798c97cdf543632a424647b901d1e214f60e0ecefb63</citedby><cites>FETCH-LOGICAL-c525t-1d13749ebde4311fda705798c97cdf543632a424647b901d1e214f60e0ecefb63</cites><orcidid>0000-0003-3616-6822 ; 0000-0003-1283-6262 ; 0000-0001-6553-4853 ; 0000-0003-2737-5681 ; 0000-0002-7065-542X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8205/825/1/L10/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,777,781,882,27905,27906,38849,38871,53821,53848</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8205/825/1/L10$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://www.osti.gov/biblio/22654290$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Osorio, Mayra</creatorcontrib><creatorcontrib>Macías, Enrique</creatorcontrib><creatorcontrib>Anglada, Guillem</creatorcontrib><creatorcontrib>Carrasco-González, Carlos</creatorcontrib><creatorcontrib>Galván-Madrid, Roberto</creatorcontrib><creatorcontrib>Zapata, Luis</creatorcontrib><creatorcontrib>Calvet, Nuria</creatorcontrib><creatorcontrib>Gómez, José F.</creatorcontrib><creatorcontrib>Nagel, Erick</creatorcontrib><creatorcontrib>Rodríguez, Luis F.</creatorcontrib><creatorcontrib>Torrelles, José M.</creatorcontrib><creatorcontrib>Zhu, Zhaohuan</creatorcontrib><title>A DWARF TRANSITIONAL PROTOPLANETARY DISK AROUND XZ TAU B</title><title>Astrophysical journal. Letters</title><addtitle>APJL</addtitle><addtitle>Astrophys. J. Lett</addtitle><description>ABSTRACT We report the discovery of a dwarf protoplanetary disk around the star XZ Tau B that shows all the features of a classical transitional disk but on a much smaller scale. The disk has been imaged with the Atacama Large Millimeter/submillimeter Array (ALMA), revealing that its dust emission has a quite small radius of ∼3.4 au and presents a central cavity of ∼1.3 au in radius that we attribute to clearing by a compact system of orbiting (proto)planets. Given the very small radii involved, evolution is expected to be much faster in this disk (observable changes in a few months) than in classical disks (observable changes requiring decades) and easy to monitor with observations in the near future. From our modeling we estimate that the mass of the disk is large enough to form a compact planetary system.</description><subject>Arrays</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>DUSTS</subject><subject>DWARF STARS</subject><subject>EMISSION</subject><subject>EVOLUTION</subject><subject>Holes</subject><subject>INTERACTIONS</subject><subject>MASS</subject><subject>MONITORS</subject><subject>Planet formation</subject><subject>planet-disk interactions</subject><subject>PLANETS</subject><subject>protoplanetary disks</subject><subject>PROTOPLANETS</subject><subject>Radio telescopes</subject><subject>SIMULATION</subject><subject>STARS</subject><subject>stars: formation</subject><subject>stars: individual (XZ Tau B)</subject><subject>stars: pre-main sequence</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNqNkMtOg0AUQInRxFr9AjckJsYNMk8YlqNtlUigoTQ-NhM6DJGGAjJ04d8LodGNiW7mTm7OuYtjGJcQ3GJGXBsBAi2GALUZoja0AwiOjMlhC_Hx9x_QU-NM6y0ACDiQTQzGzdkzjxdmEvNw5Sd-FPLAXMZREi0DHs4THr-aM3_1ZPI4Wocz8-XNTPjavDs3TvK01OriMKfGejFP7h-tIHrw73lgSYpoZ8EMYpd4apMpgiHMs9QF1PWY9FyZ5ZRgB6OUIOIQd-OBnlYIktwBCiip8o2Dp8bVeLfWXSG0LDol32VdVUp2AiGHEuSBnroZqaatP_ZKd2JXaKnKMq1UvdcCMkYgBhCxf6Cu24dyyIDiEZVtrXWrctG0xS5tPwUEYggvhqxiyNo_VEDRh-8te7SKuhHbet9WfZ8_jOtfjLTZlj-QaLIcfwF5HYlS</recordid><startdate>20160701</startdate><enddate>20160701</enddate><creator>Osorio, Mayra</creator><creator>Macías, Enrique</creator><creator>Anglada, Guillem</creator><creator>Carrasco-González, Carlos</creator><creator>Galván-Madrid, Roberto</creator><creator>Zapata, Luis</creator><creator>Calvet, Nuria</creator><creator>Gómez, José F.</creator><creator>Nagel, Erick</creator><creator>Rodríguez, Luis F.</creator><creator>Torrelles, José M.</creator><creator>Zhu, Zhaohuan</creator><general>The American Astronomical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0003-3616-6822</orcidid><orcidid>https://orcid.org/0000-0003-1283-6262</orcidid><orcidid>https://orcid.org/0000-0001-6553-4853</orcidid><orcidid>https://orcid.org/0000-0003-2737-5681</orcidid><orcidid>https://orcid.org/0000-0002-7065-542X</orcidid></search><sort><creationdate>20160701</creationdate><title>A DWARF TRANSITIONAL PROTOPLANETARY DISK AROUND XZ TAU B</title><author>Osorio, Mayra ; Macías, Enrique ; Anglada, Guillem ; Carrasco-González, Carlos ; Galván-Madrid, Roberto ; Zapata, Luis ; Calvet, Nuria ; Gómez, José F. ; Nagel, Erick ; Rodríguez, Luis F. ; Torrelles, José M. ; Zhu, Zhaohuan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c525t-1d13749ebde4311fda705798c97cdf543632a424647b901d1e214f60e0ecefb63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Arrays</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>DUSTS</topic><topic>DWARF STARS</topic><topic>EMISSION</topic><topic>EVOLUTION</topic><topic>Holes</topic><topic>INTERACTIONS</topic><topic>MASS</topic><topic>MONITORS</topic><topic>Planet formation</topic><topic>planet-disk interactions</topic><topic>PLANETS</topic><topic>protoplanetary disks</topic><topic>PROTOPLANETS</topic><topic>Radio telescopes</topic><topic>SIMULATION</topic><topic>STARS</topic><topic>stars: formation</topic><topic>stars: individual (XZ Tau B)</topic><topic>stars: pre-main sequence</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Osorio, Mayra</creatorcontrib><creatorcontrib>Macías, Enrique</creatorcontrib><creatorcontrib>Anglada, Guillem</creatorcontrib><creatorcontrib>Carrasco-González, Carlos</creatorcontrib><creatorcontrib>Galván-Madrid, Roberto</creatorcontrib><creatorcontrib>Zapata, Luis</creatorcontrib><creatorcontrib>Calvet, Nuria</creatorcontrib><creatorcontrib>Gómez, José F.</creatorcontrib><creatorcontrib>Nagel, Erick</creatorcontrib><creatorcontrib>Rodríguez, Luis F.</creatorcontrib><creatorcontrib>Torrelles, José M.</creatorcontrib><creatorcontrib>Zhu, Zhaohuan</creatorcontrib><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><collection>OSTI.GOV</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Osorio, Mayra</au><au>Macías, Enrique</au><au>Anglada, Guillem</au><au>Carrasco-González, Carlos</au><au>Galván-Madrid, Roberto</au><au>Zapata, Luis</au><au>Calvet, Nuria</au><au>Gómez, José F.</au><au>Nagel, Erick</au><au>Rodríguez, Luis F.</au><au>Torrelles, José M.</au><au>Zhu, Zhaohuan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A DWARF TRANSITIONAL PROTOPLANETARY DISK AROUND XZ TAU B</atitle><jtitle>Astrophysical journal. Letters</jtitle><stitle>APJL</stitle><addtitle>Astrophys. J. Lett</addtitle><date>2016-07-01</date><risdate>2016</risdate><volume>825</volume><issue>1</issue><spage>L10</spage><epage>L10</epage><pages>L10-L10</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>ABSTRACT We report the discovery of a dwarf protoplanetary disk around the star XZ Tau B that shows all the features of a classical transitional disk but on a much smaller scale. The disk has been imaged with the Atacama Large Millimeter/submillimeter Array (ALMA), revealing that its dust emission has a quite small radius of ∼3.4 au and presents a central cavity of ∼1.3 au in radius that we attribute to clearing by a compact system of orbiting (proto)planets. Given the very small radii involved, evolution is expected to be much faster in this disk (observable changes in a few months) than in classical disks (observable changes requiring decades) and easy to monitor with observations in the near future. From our modeling we estimate that the mass of the disk is large enough to form a compact planetary system.</abstract><cop>United States</cop><pub>The American Astronomical Society</pub><doi>10.3847/2041-8205/825/1/L10</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0003-3616-6822</orcidid><orcidid>https://orcid.org/0000-0003-1283-6262</orcidid><orcidid>https://orcid.org/0000-0001-6553-4853</orcidid><orcidid>https://orcid.org/0000-0003-2737-5681</orcidid><orcidid>https://orcid.org/0000-0002-7065-542X</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 2041-8205
ispartof Astrophysical journal. Letters, 2016-07, Vol.825 (1), p.L10-L10
issn 2041-8205
2041-8213
language eng
recordid cdi_proquest_miscellaneous_1884130128
source IOP Publishing Free Content
subjects Arrays
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
DUSTS
DWARF STARS
EMISSION
EVOLUTION
Holes
INTERACTIONS
MASS
MONITORS
Planet formation
planet-disk interactions
PLANETS
protoplanetary disks
PROTOPLANETS
Radio telescopes
SIMULATION
STARS
stars: formation
stars: individual (XZ Tau B)
stars: pre-main sequence
title A DWARF TRANSITIONAL PROTOPLANETARY DISK AROUND XZ TAU B
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-20T17%3A58%3A15IST&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%20DWARF%20TRANSITIONAL%20PROTOPLANETARY%20DISK%20AROUND%20XZ%20TAU%20B&rft.jtitle=Astrophysical%20journal.%20Letters&rft.au=Osorio,%20Mayra&rft.date=2016-07-01&rft.volume=825&rft.issue=1&rft.spage=L10&rft.epage=L10&rft.pages=L10-L10&rft.issn=2041-8205&rft.eissn=2041-8213&rft_id=info:doi/10.3847/2041-8205/825/1/L10&rft_dat=%3Cproquest_O3W%3E1884130128%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=1877820648&rft_id=info:pmid/&rfr_iscdi=true