ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527
- Autores
- Harris, Robert J.; Cox, Erin G.; Looney, Leslie W.; Li, Zhi-Yun; Yang, Haifeng; Fernandez Lopez, Manuel; Kwon, Woojin; Sadavoy, Sarah; Segura Cox, Dominique; Stephens, Ian; Tobin, John
- Año de publicación
- 2018
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present high-sensitivity (σ I ∼ 0.2-0.5 mJy, σ QU ∼ 0.05 mJy), high-resolution (∼0.″12 -0.″2) observations of polarized 872 μm dust emission from the young multiple system VLA 1623 in ρ Ophiuchus and the protostar L1527 in Taurus. We detect the circumstellar material of VLA 1623A, the extended Keplerian disk surrounding VLA 1623A that we call VLA 1623CBdisk, VLA 1623B, VLA 1623W, and L1527 strongly in the polarized emission, at the ∼1%-3% level. We spatially resolve VLA 1623A into two sources, VLA 1623Aa and VLA 1623Ab, separated by ∼30 au and located within a cavity of radius ∼50 au within the circumbinary Keplerian disk, as well as the edge-on disk of VLA 1623W. The polarization angle of the emission is uniform across each protostellar source and nearly coincides with each disk's minor axis. The offsets between the minor axis position angle and the polarization angle are not uniformly distributed at the P ≲ 2 ×10-4 level. The circumbinary disk surrounding VLA 1623Aab is azimuthally symmetrically polarized. Each compact source's emission is partially optically thick (τ 1) at 872 μm, complicating interpretations of polarization involving aligned grains. We find evidence against alignment by radiative flux in each source, particularly in the edge-on VLA 1623W and L1527. We detect astrometric offsets between the polarized emission and the total intensity in VLA 1623Aa, VLA 1623Ab, and VLA 1623B, as predicted if self-scattering in the optically thick limit operates. We conclude that self-scattering is likely responsible for disk-scale polarization at 872 μm in these systems.
Fil: Harris, Robert J.. University of Illinois. Urbana - Champaign; Estados Unidos
Fil: Cox, Erin G.. University of Illinois. Urbana - Champaign; Estados Unidos
Fil: Looney, Leslie W.. University of Illinois. Urbana - Champaign; Estados Unidos
Fil: Li, Zhi-Yun. University of Virginia; Estados Unidos
Fil: Yang, Haifeng. University of Virginia; Estados Unidos
Fil: Fernandez Lopez, Manuel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Kwon, Woojin. Korea Astronomy And Space Science Institute; Corea del Sur
Fil: Sadavoy, Sarah. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Segura Cox, Dominique. University of Illinois. Urbana - Champaign; Estados Unidos
Fil: Stephens, Ian. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Tobin, John. Oklahoma State University; Estados Unidos. Leiden University; Países Bajos - Materia
-
CIRCUMSTELLAR MATTER
SCATTERING
STARS: FORMATION
STARS: MAGNETIC FIELD - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/82424
Ver los metadatos del registro completo
id |
CONICETDig_d75c00532325686a51c0bc415f7b446f |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/82424 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527Harris, Robert J.Cox, Erin G.Looney, Leslie W.Li, Zhi-YunYang, HaifengFernandez Lopez, ManuelKwon, WoojinSadavoy, SarahSegura Cox, DominiqueStephens, IanTobin, JohnCIRCUMSTELLAR MATTERSCATTERINGSTARS: FORMATIONSTARS: MAGNETIC FIELDhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present high-sensitivity (σ I ∼ 0.2-0.5 mJy, σ QU ∼ 0.05 mJy), high-resolution (∼0.″12 -0.″2) observations of polarized 872 μm dust emission from the young multiple system VLA 1623 in ρ Ophiuchus and the protostar L1527 in Taurus. We detect the circumstellar material of VLA 1623A, the extended Keplerian disk surrounding VLA 1623A that we call VLA 1623CBdisk, VLA 1623B, VLA 1623W, and L1527 strongly in the polarized emission, at the ∼1%-3% level. We spatially resolve VLA 1623A into two sources, VLA 1623Aa and VLA 1623Ab, separated by ∼30 au and located within a cavity of radius ∼50 au within the circumbinary Keplerian disk, as well as the edge-on disk of VLA 1623W. The polarization angle of the emission is uniform across each protostellar source and nearly coincides with each disk's minor axis. The offsets between the minor axis position angle and the polarization angle are not uniformly distributed at the P ≲ 2 ×10-4 level. The circumbinary disk surrounding VLA 1623Aab is azimuthally symmetrically polarized. Each compact source's emission is partially optically thick (τ 1) at 872 μm, complicating interpretations of polarization involving aligned grains. We find evidence against alignment by radiative flux in each source, particularly in the edge-on VLA 1623W and L1527. We detect astrometric offsets between the polarized emission and the total intensity in VLA 1623Aa, VLA 1623Ab, and VLA 1623B, as predicted if self-scattering in the optically thick limit operates. We conclude that self-scattering is likely responsible for disk-scale polarization at 872 μm in these systems.Fil: Harris, Robert J.. University of Illinois. Urbana - Champaign; Estados UnidosFil: Cox, Erin G.. University of Illinois. Urbana - Champaign; Estados UnidosFil: Looney, Leslie W.. University of Illinois. Urbana - Champaign; Estados UnidosFil: Li, Zhi-Yun. University of Virginia; Estados UnidosFil: Yang, Haifeng. University of Virginia; Estados UnidosFil: Fernandez Lopez, Manuel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Kwon, Woojin. Korea Astronomy And Space Science Institute; Corea del SurFil: Sadavoy, Sarah. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Segura Cox, Dominique. University of Illinois. Urbana - Champaign; Estados UnidosFil: Stephens, Ian. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Tobin, John. Oklahoma State University; Estados Unidos. Leiden University; Países BajosIOP Publishing2018-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/82424Harris, Robert J.; Cox, Erin G.; Looney, Leslie W.; Li, Zhi-Yun; Yang, Haifeng; et al.; ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527; IOP Publishing; Astrophysical Journal; 861; 2; 7-2018; 1-220004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aac6ecinfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/aac6ecinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:42:04Zoai:ri.conicet.gov.ar:11336/82424instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:42:04.516CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 |
title |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 |
spellingShingle |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 Harris, Robert J. CIRCUMSTELLAR MATTER SCATTERING STARS: FORMATION STARS: MAGNETIC FIELD |
title_short |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 |
title_full |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 |
title_fullStr |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 |
title_full_unstemmed |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 |
title_sort |
ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527 |
dc.creator.none.fl_str_mv |
Harris, Robert J. Cox, Erin G. Looney, Leslie W. Li, Zhi-Yun Yang, Haifeng Fernandez Lopez, Manuel Kwon, Woojin Sadavoy, Sarah Segura Cox, Dominique Stephens, Ian Tobin, John |
author |
Harris, Robert J. |
author_facet |
Harris, Robert J. Cox, Erin G. Looney, Leslie W. Li, Zhi-Yun Yang, Haifeng Fernandez Lopez, Manuel Kwon, Woojin Sadavoy, Sarah Segura Cox, Dominique Stephens, Ian Tobin, John |
author_role |
author |
author2 |
Cox, Erin G. Looney, Leslie W. Li, Zhi-Yun Yang, Haifeng Fernandez Lopez, Manuel Kwon, Woojin Sadavoy, Sarah Segura Cox, Dominique Stephens, Ian Tobin, John |
author2_role |
author author author author author author author author author author |
dc.subject.none.fl_str_mv |
CIRCUMSTELLAR MATTER SCATTERING STARS: FORMATION STARS: MAGNETIC FIELD |
topic |
CIRCUMSTELLAR MATTER SCATTERING STARS: FORMATION STARS: MAGNETIC FIELD |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We present high-sensitivity (σ I ∼ 0.2-0.5 mJy, σ QU ∼ 0.05 mJy), high-resolution (∼0.″12 -0.″2) observations of polarized 872 μm dust emission from the young multiple system VLA 1623 in ρ Ophiuchus and the protostar L1527 in Taurus. We detect the circumstellar material of VLA 1623A, the extended Keplerian disk surrounding VLA 1623A that we call VLA 1623CBdisk, VLA 1623B, VLA 1623W, and L1527 strongly in the polarized emission, at the ∼1%-3% level. We spatially resolve VLA 1623A into two sources, VLA 1623Aa and VLA 1623Ab, separated by ∼30 au and located within a cavity of radius ∼50 au within the circumbinary Keplerian disk, as well as the edge-on disk of VLA 1623W. The polarization angle of the emission is uniform across each protostellar source and nearly coincides with each disk's minor axis. The offsets between the minor axis position angle and the polarization angle are not uniformly distributed at the P ≲ 2 ×10-4 level. The circumbinary disk surrounding VLA 1623Aab is azimuthally symmetrically polarized. Each compact source's emission is partially optically thick (τ 1) at 872 μm, complicating interpretations of polarization involving aligned grains. We find evidence against alignment by radiative flux in each source, particularly in the edge-on VLA 1623W and L1527. We detect astrometric offsets between the polarized emission and the total intensity in VLA 1623Aa, VLA 1623Ab, and VLA 1623B, as predicted if self-scattering in the optically thick limit operates. We conclude that self-scattering is likely responsible for disk-scale polarization at 872 μm in these systems. Fil: Harris, Robert J.. University of Illinois. Urbana - Champaign; Estados Unidos Fil: Cox, Erin G.. University of Illinois. Urbana - Champaign; Estados Unidos Fil: Looney, Leslie W.. University of Illinois. Urbana - Champaign; Estados Unidos Fil: Li, Zhi-Yun. University of Virginia; Estados Unidos Fil: Yang, Haifeng. University of Virginia; Estados Unidos Fil: Fernandez Lopez, Manuel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Kwon, Woojin. Korea Astronomy And Space Science Institute; Corea del Sur Fil: Sadavoy, Sarah. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Segura Cox, Dominique. University of Illinois. Urbana - Champaign; Estados Unidos Fil: Stephens, Ian. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Tobin, John. Oklahoma State University; Estados Unidos. Leiden University; Países Bajos |
description |
We present high-sensitivity (σ I ∼ 0.2-0.5 mJy, σ QU ∼ 0.05 mJy), high-resolution (∼0.″12 -0.″2) observations of polarized 872 μm dust emission from the young multiple system VLA 1623 in ρ Ophiuchus and the protostar L1527 in Taurus. We detect the circumstellar material of VLA 1623A, the extended Keplerian disk surrounding VLA 1623A that we call VLA 1623CBdisk, VLA 1623B, VLA 1623W, and L1527 strongly in the polarized emission, at the ∼1%-3% level. We spatially resolve VLA 1623A into two sources, VLA 1623Aa and VLA 1623Ab, separated by ∼30 au and located within a cavity of radius ∼50 au within the circumbinary Keplerian disk, as well as the edge-on disk of VLA 1623W. The polarization angle of the emission is uniform across each protostellar source and nearly coincides with each disk's minor axis. The offsets between the minor axis position angle and the polarization angle are not uniformly distributed at the P ≲ 2 ×10-4 level. The circumbinary disk surrounding VLA 1623Aab is azimuthally symmetrically polarized. Each compact source's emission is partially optically thick (τ 1) at 872 μm, complicating interpretations of polarization involving aligned grains. We find evidence against alignment by radiative flux in each source, particularly in the edge-on VLA 1623W and L1527. We detect astrometric offsets between the polarized emission and the total intensity in VLA 1623Aa, VLA 1623Ab, and VLA 1623B, as predicted if self-scattering in the optically thick limit operates. We conclude that self-scattering is likely responsible for disk-scale polarization at 872 μm in these systems. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-07 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/82424 Harris, Robert J.; Cox, Erin G.; Looney, Leslie W.; Li, Zhi-Yun; Yang, Haifeng; et al.; ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527; IOP Publishing; Astrophysical Journal; 861; 2; 7-2018; 1-22 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/82424 |
identifier_str_mv |
Harris, Robert J.; Cox, Erin G.; Looney, Leslie W.; Li, Zhi-Yun; Yang, Haifeng; et al.; ALMA Observations of Polarized 872 μm Dust Emission from the Protostellar Systems VLA 1623 and L1527; IOP Publishing; Astrophysical Journal; 861; 2; 7-2018; 1-22 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aac6ec info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/aac6ec |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
_version_ |
1844614452946665472 |
score |
13.070432 |