Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey

Context. Complex organic molecules (COMs) have been detected in a few Class 0 protostars but their origin is not well understood. While the usual picture of a hot corino explains their presence as resulting from the heating of the inner envelope by the nascent protostar, shocks in the outflow, disk...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2020-03, Vol.635, p.A198
Hauptverfasser: Belloche, A., Maury, A. J., Maret, S., Anderl, S., Bacmann, A., André, Ph, Bontemps, S., Cabrit, S., Codella, C., Gaudel, M., Gueth, F., Lefèvre, C., Lefloch, B., Podio, L., Testi, L.
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container_issue
container_start_page A198
container_title Astronomy and astrophysics (Berlin)
container_volume 635
creator Belloche, A.
Maury, A. J.
Maret, S.
Anderl, S.
Bacmann, A.
André, Ph
Bontemps, S.
Cabrit, S.
Codella, C.
Gaudel, M.
Gueth, F.
Lefèvre, C.
Lefloch, B.
Podio, L.
Testi, L.
description Context. Complex organic molecules (COMs) have been detected in a few Class 0 protostars but their origin is not well understood. While the usual picture of a hot corino explains their presence as resulting from the heating of the inner envelope by the nascent protostar, shocks in the outflow, disk wind, the presence of a flared disk, or the interaction region between envelope and disk at the centrifugal barrier have also been claimed to enhance the abundance of COMs. Aims. Going beyond studies of individual objects, we want to investigate the origin of COMs in young protostars on a statistical basis. Methods. We use the CALYPSO survey performed with the Plateau de Bure Interferometer of the Institut de Radioastronomie Millimétrique to search for COMs at high angular resolution in a sample of 26 solar-type protostars, including 22 Class 0 and four Class I objects. We derive the column densities of the detected molecules under the local thermodynamic equilibrium approximation and search for correlations between their abundances and with various source properties. Results. Methanol is detected in 12 sources and tentatively in one source, which represents half of the sample. Eight sources (30%) have detections of at least three COMs. We find a strong chemical differentiation in multiple systems with five systems having one component with at least three COMs detected but the other component devoid of COM emission. All sources with a luminosity higher than 4 L ⊙ have at least one detected COM whereas no COM emission is detected in sources with internal luminosity lower than 2 L ⊙ , likely because of a lack of sensitivity. Internal luminosity is found to be the source parameter impacting the COM chemical composition of the sources the most, while there is no obvious correlation between the detection of COM emission and that of a disk-like structure. A canonical hot-corino origin may explain the COM emission in four sources, an accretion-shock origin in two or possibly three sources, and an outflow origin in three sources. The CALYPSO sources with COM detections can be classified into three groups on the basis of the abundances of oxygen-bearing molecules, cyanides, and CHO-bearing molecules. These chemical groups correlate neither with the COM origin scenarios, nor with the evolutionary status of the sources if we take the ratio of envelope mass to internal luminosity as an evolutionary tracer. We find strong correlations between molecules that are a priori not
doi_str_mv 10.1051/0004-6361/201937352
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J. ; Maret, S. ; Anderl, S. ; Bacmann, A. ; André, Ph ; Bontemps, S. ; Cabrit, S. ; Codella, C. ; Gaudel, M. ; Gueth, F. ; Lefèvre, C. ; Lefloch, B. ; Podio, L. ; Testi, L.</creator><creatorcontrib>Belloche, A. ; Maury, A. J. ; Maret, S. ; Anderl, S. ; Bacmann, A. ; André, Ph ; Bontemps, S. ; Cabrit, S. ; Codella, C. ; Gaudel, M. ; Gueth, F. ; Lefèvre, C. ; Lefloch, B. ; Podio, L. ; Testi, L.</creatorcontrib><description>Context. Complex organic molecules (COMs) have been detected in a few Class 0 protostars but their origin is not well understood. While the usual picture of a hot corino explains their presence as resulting from the heating of the inner envelope by the nascent protostar, shocks in the outflow, disk wind, the presence of a flared disk, or the interaction region between envelope and disk at the centrifugal barrier have also been claimed to enhance the abundance of COMs. Aims. Going beyond studies of individual objects, we want to investigate the origin of COMs in young protostars on a statistical basis. Methods. We use the CALYPSO survey performed with the Plateau de Bure Interferometer of the Institut de Radioastronomie Millimétrique to search for COMs at high angular resolution in a sample of 26 solar-type protostars, including 22 Class 0 and four Class I objects. We derive the column densities of the detected molecules under the local thermodynamic equilibrium approximation and search for correlations between their abundances and with various source properties. Results. Methanol is detected in 12 sources and tentatively in one source, which represents half of the sample. Eight sources (30%) have detections of at least three COMs. We find a strong chemical differentiation in multiple systems with five systems having one component with at least three COMs detected but the other component devoid of COM emission. All sources with a luminosity higher than 4 L ⊙ have at least one detected COM whereas no COM emission is detected in sources with internal luminosity lower than 2 L ⊙ , likely because of a lack of sensitivity. Internal luminosity is found to be the source parameter impacting the COM chemical composition of the sources the most, while there is no obvious correlation between the detection of COM emission and that of a disk-like structure. A canonical hot-corino origin may explain the COM emission in four sources, an accretion-shock origin in two or possibly three sources, and an outflow origin in three sources. The CALYPSO sources with COM detections can be classified into three groups on the basis of the abundances of oxygen-bearing molecules, cyanides, and CHO-bearing molecules. These chemical groups correlate neither with the COM origin scenarios, nor with the evolutionary status of the sources if we take the ratio of envelope mass to internal luminosity as an evolutionary tracer. We find strong correlations between molecules that are a priori not related chemically (for instance methanol and methyl cyanide), implying that the existence of a correlation does not imply a chemical link. Conclusions. The CALYPSO survey has revealed a chemical differentiation in multiple systems that is markedly different from the case of the prototypical binary IRAS 16293-2422. This raises the question of whether all low-mass protostars go through a phase showing COM emission. A larger sample of young protostars and a more accurate determination of their internal luminosity will be necessary to make further progress. Searching for correlations between the COM emission and the jet/outflow properties of the sources may also be promising.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>EISSN: 1432-0756</identifier><identifier>DOI: 10.1051/0004-6361/201937352</identifier><language>eng</language><publisher>Heidelberg: EDP Sciences</publisher><subject>Abundance ; Acetonitrile ; Angular resolution ; Astrophysics ; Chemical composition ; Correlation ; Deposition ; Differentiation ; Emission ; Local thermodynamic equilibrium ; Luminosity ; Methanol ; Object recognition ; Organic chemistry ; Outflow ; Parameter sensitivity ; Physics ; Protostars ; Questions ; Statistical methods</subject><ispartof>Astronomy and astrophysics (Berlin), 2020-03, Vol.635, p.A198</ispartof><rights>2020. This work is licensed under http://creativecommons.org/licenses/by/4.0 (the “License”). Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the terms of the License.</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-c2712-1d3dfc37ccbb30673af9cea604e9fa067fd36b00832a64dc2860fa9d2eaa74073</citedby><cites>FETCH-LOGICAL-c2712-1d3dfc37ccbb30673af9cea604e9fa067fd36b00832a64dc2860fa9d2eaa74073</cites><orcidid>0000-0003-0046-6217 ; 0000-0003-1263-4986 ; 0000-0003-2733-5372 ; 0000-0003-1104-4554 ; 0000-0002-5482-5206 ; 0000-0002-1593-3693 ; 0000-0003-1859-3070 ; 0000-0001-7349-6113 ; 0000-0003-1514-3074 ; 0000-0002-9397-3826 ; 0000-0002-4093-7178</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,3726,27923,27924</link.rule.ids><backlink>$$Uhttps://cea.hal.science/cea-02534276$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Belloche, A.</creatorcontrib><creatorcontrib>Maury, A. J.</creatorcontrib><creatorcontrib>Maret, S.</creatorcontrib><creatorcontrib>Anderl, S.</creatorcontrib><creatorcontrib>Bacmann, A.</creatorcontrib><creatorcontrib>André, Ph</creatorcontrib><creatorcontrib>Bontemps, S.</creatorcontrib><creatorcontrib>Cabrit, S.</creatorcontrib><creatorcontrib>Codella, C.</creatorcontrib><creatorcontrib>Gaudel, M.</creatorcontrib><creatorcontrib>Gueth, F.</creatorcontrib><creatorcontrib>Lefèvre, C.</creatorcontrib><creatorcontrib>Lefloch, B.</creatorcontrib><creatorcontrib>Podio, L.</creatorcontrib><creatorcontrib>Testi, L.</creatorcontrib><title>Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey</title><title>Astronomy and astrophysics (Berlin)</title><description>Context. Complex organic molecules (COMs) have been detected in a few Class 0 protostars but their origin is not well understood. While the usual picture of a hot corino explains their presence as resulting from the heating of the inner envelope by the nascent protostar, shocks in the outflow, disk wind, the presence of a flared disk, or the interaction region between envelope and disk at the centrifugal barrier have also been claimed to enhance the abundance of COMs. Aims. Going beyond studies of individual objects, we want to investigate the origin of COMs in young protostars on a statistical basis. Methods. We use the CALYPSO survey performed with the Plateau de Bure Interferometer of the Institut de Radioastronomie Millimétrique to search for COMs at high angular resolution in a sample of 26 solar-type protostars, including 22 Class 0 and four Class I objects. We derive the column densities of the detected molecules under the local thermodynamic equilibrium approximation and search for correlations between their abundances and with various source properties. Results. Methanol is detected in 12 sources and tentatively in one source, which represents half of the sample. Eight sources (30%) have detections of at least three COMs. We find a strong chemical differentiation in multiple systems with five systems having one component with at least three COMs detected but the other component devoid of COM emission. All sources with a luminosity higher than 4 L ⊙ have at least one detected COM whereas no COM emission is detected in sources with internal luminosity lower than 2 L ⊙ , likely because of a lack of sensitivity. Internal luminosity is found to be the source parameter impacting the COM chemical composition of the sources the most, while there is no obvious correlation between the detection of COM emission and that of a disk-like structure. A canonical hot-corino origin may explain the COM emission in four sources, an accretion-shock origin in two or possibly three sources, and an outflow origin in three sources. The CALYPSO sources with COM detections can be classified into three groups on the basis of the abundances of oxygen-bearing molecules, cyanides, and CHO-bearing molecules. These chemical groups correlate neither with the COM origin scenarios, nor with the evolutionary status of the sources if we take the ratio of envelope mass to internal luminosity as an evolutionary tracer. We find strong correlations between molecules that are a priori not related chemically (for instance methanol and methyl cyanide), implying that the existence of a correlation does not imply a chemical link. Conclusions. The CALYPSO survey has revealed a chemical differentiation in multiple systems that is markedly different from the case of the prototypical binary IRAS 16293-2422. This raises the question of whether all low-mass protostars go through a phase showing COM emission. A larger sample of young protostars and a more accurate determination of their internal luminosity will be necessary to make further progress. Searching for correlations between the COM emission and the jet/outflow properties of the sources may also be promising.</description><subject>Abundance</subject><subject>Acetonitrile</subject><subject>Angular resolution</subject><subject>Astrophysics</subject><subject>Chemical composition</subject><subject>Correlation</subject><subject>Deposition</subject><subject>Differentiation</subject><subject>Emission</subject><subject>Local thermodynamic equilibrium</subject><subject>Luminosity</subject><subject>Methanol</subject><subject>Object recognition</subject><subject>Organic chemistry</subject><subject>Outflow</subject><subject>Parameter sensitivity</subject><subject>Physics</subject><subject>Protostars</subject><subject>Questions</subject><subject>Statistical methods</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>eNo9kE1LAzEQhoMoWKu_wEvAk4e1-dpk91iKWqGgoh48hTSbtCnbzZrsVvvvzVrpaZiZZ16GB4BrjO4wyvEEIcQyTjmeEIRLKmhOTsAIM0oyJBg_BaMjcQ4uYtykluCCjsDqtTexc75xzQp2awNjqzqnauiDW7kGegu137a1-UmTlWqchltfG93XJsK03_s-HbbBdz52KkT47br1X9Bsuvh8eXuGsQ87s78EZ1bV0Vz91zH4eLh_n82zxfPjU0IzTQQmGa5oZTUVWi-XFHFBlS21URwxU1qVBraifIlQQYnirNKk4MiqsiJGKcGQoGNwe8hdq1q2wW1V2EuvnJxPFzIlSURyyojgO5zYmwOb3v8aNMiN70OT3pOEFQJjVpR5ouiB0sHHGIw9xmIkB_tycCsHt_Jon_4CAWB3gQ</recordid><startdate>20200301</startdate><enddate>20200301</enddate><creator>Belloche, A.</creator><creator>Maury, A. 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J. ; Maret, S. ; Anderl, S. ; Bacmann, A. ; André, Ph ; Bontemps, S. ; Cabrit, S. ; Codella, C. ; Gaudel, M. ; Gueth, F. ; Lefèvre, C. ; Lefloch, B. ; Podio, L. ; Testi, L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2712-1d3dfc37ccbb30673af9cea604e9fa067fd36b00832a64dc2860fa9d2eaa74073</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Abundance</topic><topic>Acetonitrile</topic><topic>Angular resolution</topic><topic>Astrophysics</topic><topic>Chemical composition</topic><topic>Correlation</topic><topic>Deposition</topic><topic>Differentiation</topic><topic>Emission</topic><topic>Local thermodynamic equilibrium</topic><topic>Luminosity</topic><topic>Methanol</topic><topic>Object recognition</topic><topic>Organic chemistry</topic><topic>Outflow</topic><topic>Parameter sensitivity</topic><topic>Physics</topic><topic>Protostars</topic><topic>Questions</topic><topic>Statistical methods</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Belloche, A.</creatorcontrib><creatorcontrib>Maury, A. 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J.</au><au>Maret, S.</au><au>Anderl, S.</au><au>Bacmann, A.</au><au>André, Ph</au><au>Bontemps, S.</au><au>Cabrit, S.</au><au>Codella, C.</au><au>Gaudel, M.</au><au>Gueth, F.</au><au>Lefèvre, C.</au><au>Lefloch, B.</au><au>Podio, L.</au><au>Testi, L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2020-03-01</date><risdate>2020</risdate><volume>635</volume><spage>A198</spage><pages>A198-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><eissn>1432-0756</eissn><abstract>Context. Complex organic molecules (COMs) have been detected in a few Class 0 protostars but their origin is not well understood. While the usual picture of a hot corino explains their presence as resulting from the heating of the inner envelope by the nascent protostar, shocks in the outflow, disk wind, the presence of a flared disk, or the interaction region between envelope and disk at the centrifugal barrier have also been claimed to enhance the abundance of COMs. Aims. Going beyond studies of individual objects, we want to investigate the origin of COMs in young protostars on a statistical basis. Methods. We use the CALYPSO survey performed with the Plateau de Bure Interferometer of the Institut de Radioastronomie Millimétrique to search for COMs at high angular resolution in a sample of 26 solar-type protostars, including 22 Class 0 and four Class I objects. We derive the column densities of the detected molecules under the local thermodynamic equilibrium approximation and search for correlations between their abundances and with various source properties. Results. Methanol is detected in 12 sources and tentatively in one source, which represents half of the sample. Eight sources (30%) have detections of at least three COMs. We find a strong chemical differentiation in multiple systems with five systems having one component with at least three COMs detected but the other component devoid of COM emission. All sources with a luminosity higher than 4 L ⊙ have at least one detected COM whereas no COM emission is detected in sources with internal luminosity lower than 2 L ⊙ , likely because of a lack of sensitivity. Internal luminosity is found to be the source parameter impacting the COM chemical composition of the sources the most, while there is no obvious correlation between the detection of COM emission and that of a disk-like structure. A canonical hot-corino origin may explain the COM emission in four sources, an accretion-shock origin in two or possibly three sources, and an outflow origin in three sources. The CALYPSO sources with COM detections can be classified into three groups on the basis of the abundances of oxygen-bearing molecules, cyanides, and CHO-bearing molecules. These chemical groups correlate neither with the COM origin scenarios, nor with the evolutionary status of the sources if we take the ratio of envelope mass to internal luminosity as an evolutionary tracer. We find strong correlations between molecules that are a priori not related chemically (for instance methanol and methyl cyanide), implying that the existence of a correlation does not imply a chemical link. Conclusions. The CALYPSO survey has revealed a chemical differentiation in multiple systems that is markedly different from the case of the prototypical binary IRAS 16293-2422. This raises the question of whether all low-mass protostars go through a phase showing COM emission. 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subjects Abundance
Acetonitrile
Angular resolution
Astrophysics
Chemical composition
Correlation
Deposition
Differentiation
Emission
Local thermodynamic equilibrium
Luminosity
Methanol
Object recognition
Organic chemistry
Outflow
Parameter sensitivity
Physics
Protostars
Questions
Statistical methods
title Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey
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