The Herschel and JCMT Gould Belt Surveys: Constraining Dust Properties in the Perseus B1 Clump with PACS, SPIRE, and SCUBA-2
| dc.contributor.author | SADAVOY, S. I. | |
| hal.structure.identifier | Herzberg Institute of Astrophysics | |
| dc.contributor.author | DI FRANCESCO, J. | |
| hal.structure.identifier | Natl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7 Canada | |
| dc.contributor.author | JOHNSTONE, D. | |
| dc.contributor.author | CURRIE, M. J. | |
| dc.contributor.author | DRABEK, E. | |
| dc.contributor.author | HATCHELL, J. | |
| hal.structure.identifier | School of Physics and Astronomy [Cardiff] | |
| dc.contributor.author | NUTTER, D. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | ANDRÉ, Ph. | |
| dc.contributor.author | ARZOUMANIAN, D. | |
| hal.structure.identifier | Institut de Planétologie et d'Astrophysique de Grenoble [IPAG] | |
| dc.contributor.author | BENEDETTINI, M. | |
| dc.contributor.author | BERNARD, J. -P. | |
| hal.structure.identifier | FORMATION STELLAIRE 2013 | |
| dc.contributor.author | DUARTE-CABRAL, A. | |
| dc.contributor.author | FALLSCHEER, C. | |
| dc.contributor.author | FRIESEN, R. | |
| hal.structure.identifier | Opération Cétacés | |
| dc.contributor.author | GREAVES, J. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | HENNEMANN, M. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | HILL, T. | |
| dc.contributor.author | JENNESS, T. | |
| dc.contributor.author | KÖNYVES, V. | |
| dc.contributor.author | MATTHEWS, B. | |
| dc.contributor.author | MOTTRAM, J. C. | |
| hal.structure.identifier | Istituto di Fisica dello Spazio Interplanetario [IFSI] | |
| dc.contributor.author | PEZZUTO, S. | |
| hal.structure.identifier | Milieux aquatiques, écologie et pollutions [UR MALY] | |
| dc.contributor.author | ROY, A. | |
| dc.contributor.author | RYGL, K. | |
| hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
| hal.structure.identifier | Université Sciences et Technologies - Bordeaux 1 [UB] | |
| hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
| hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
| dc.contributor.author | SCHNEIDER, N. | |
| hal.structure.identifier | Antarctic Research a European Network for Astrophysics [ARENA] | |
| dc.contributor.author | SPINOGLIO, L. | |
| hal.structure.identifier | European Southern Observatory [ESO] | |
| dc.contributor.author | TESTI, L. | |
| hal.structure.identifier | Antarctic Research a European Network for Astrophysics [ARENA] | |
| dc.contributor.author | TOTHILL, N. | |
| hal.structure.identifier | School of Physics and Astronomy [Cardiff] | |
| dc.contributor.author | WARD-THOMPSON, D. | |
| hal.structure.identifier | STFC Rutherford Appleton Laboratory [RAL] | |
| dc.contributor.author | WHITE, G. | |
| dc.date.created | 2013-03-06 | |
| dc.date.issued | 2013 | |
| dc.identifier.issn | 0004-637X | |
| dc.description.abstractEn | We present Herschel observations from the Herschel Gould Belt Survey and SCUBA-2 science verification observations from the JCMT Gould Belt Survey of the B1 clump in the Perseus molecular cloud. We determined the dust emissivity index using four different techniques to combine the Herschel PACS+SPIRE data at 160 - 500 microns with the SCUBA-2 data at 450 microns and 850 microns. Of our four techniques, we found the most robust method was to filter-out the large-scale emission in the Herschel bands to match the spatial scales recovered by the SCUBA-2 reduction pipeline. Using this method, we find beta ~ 2 towards the filament region and moderately dense material and lower beta values (beta > 1.6) towards the dense protostellar cores, possibly due to dust grain growth. We find that beta and temperature are more robust with the inclusion of the SCUBA-2 data, improving estimates from Herschel data alone by factors of ~ 2 for beta and by ~ 40% for temperature. Furthermore, we find core mass differences of < 30% compared to Herschel-only estimates with an adopted beta = 2, highlighting the necessity of long wavelength submillimeter data for deriving accurate masses of prestellar and protostellar cores. | |
| dc.language.iso | en | |
| dc.publisher | American Astronomical Society | |
| dc.subject.en | dust | |
| dc.subject.en | extinction | |
| dc.subject.en | ISM: clouds | |
| dc.subject.en | stars: formation | |
| dc.subject.en | stars: low-mass | |
| dc.subject.en | stars: protostars | |
| dc.title.en | The Herschel and JCMT Gould Belt Surveys: Constraining Dust Properties in the Perseus B1 Clump with PACS, SPIRE, and SCUBA-2 | |
| dc.type | Article de revue | |
| dc.identifier.doi | 10.1088/0004-637X/767/2/126 | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.identifier.arxiv | 1303.1529 | |
| bordeaux.journal | The Astrophysical Journal | |
| bordeaux.page | id. 126 | |
| bordeaux.volume | 767 | |
| bordeaux.issue | 2 | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-00824698 | |
| hal.version | 1 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-00824698v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=The%20Astrophysical%20Journal&rft.date=2013&rft.volume=767&rft.issue=2&rft.spage=id.%20126&rft.epage=id.%20126&rft.eissn=0004-637X&rft.issn=0004-637X&rft.au=SADAVOY,%20S.%20I.&DI%20FRANCESCO,%20J.&JOHNSTONE,%20D.&CURRIE,%20M.%20J.&DRABEK,%20E.&rft.genre=article |
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