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Article: The discovery based on GLIMPSE data of a protostar driving a bipolar outflow

TitleThe discovery based on GLIMPSE data of a protostar driving a bipolar outflow
Authors
Yuan, JLi, ZHuang, YHsia, CMiao, J
KeywordsClass i
Color-color diagrams
Driving source
Evolutionary stage
In-line
Issue Date2012
PublisherEDP Sciences. The Journal's web site is located at http://www.aanda.org
Citation
Astronomy & Astrophysics, 2012, v. 540, article no. A95 How to Cite?
DOI: http://dx.doi.org/10.1051/0004-6361/201117858
AbstractWe report the discovery based on GLIMPSE data of a proto-stellar system driving a bipolar outflow. The bipolar outflow closely resembles the shape of an hourglass in the infrared. The total luminosity of L total = 5507 L ̇, derived from IRAS fluxes, indicates the ongoing formation of a massive star in this region. The spectral energy distribution (SED) of the driving source is fitted with an online SED fitting tool, which results in a spectral index of about 1.2. This, along with the presence of a bipolar outflow, suggests the detection of a Class I protostar. The driving source indicates prominent infrared excesses in color-color diagrams based on archived 2 MASS and GLIMPSE data, which is in line with an early evolutionary stage of the system. © 2012 ESO.
Persistent Identifierhttp://hdl.handle.net/10722/164513
ISSN
0004-6361
2023 Impact Factor: 5.4
2023 SCImago Journal Rankings: 1.896
ISI Accession Number ID
WOS:000303315400109
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorYuan, Jen_HK
dc.contributor.authorLi, Zen_HK
dc.contributor.authorHuang, Yen_HK
dc.contributor.authorHsia, Cen_HK
dc.contributor.authorMiao, Jen_HK
dc.date.accessioned2012-09-20T08:04:51Z-
dc.date.available2012-09-20T08:04:51Z-
dc.date.issued2012en_HK
dc.identifier.citationAstronomy & Astrophysics, 2012, v. 540, article no. A95en_HK
dc.identifier.issn0004-6361en_HK
dc.identifier.urihttp://hdl.handle.net/10722/164513-
dc.description.abstractWe report the discovery based on GLIMPSE data of a proto-stellar system driving a bipolar outflow. The bipolar outflow closely resembles the shape of an hourglass in the infrared. The total luminosity of L total = 5507 L ̇, derived from IRAS fluxes, indicates the ongoing formation of a massive star in this region. The spectral energy distribution (SED) of the driving source is fitted with an online SED fitting tool, which results in a spectral index of about 1.2. This, along with the presence of a bipolar outflow, suggests the detection of a Class I protostar. The driving source indicates prominent infrared excesses in color-color diagrams based on archived 2 MASS and GLIMPSE data, which is in line with an early evolutionary stage of the system. © 2012 ESO.en_HK
dc.languageengen_US
dc.publisherEDP Sciences. The Journal's web site is located at http://www.aanda.orgen_HK
dc.relation.ispartofAstronomy & Astrophysicsen_HK
dc.rightsThe original publication is available at [http://www.aanda.org/]-
dc.subjectClass ien_HK
dc.subjectColor-color diagramsen_HK
dc.subjectDriving sourceen_HK
dc.subjectEvolutionary stageen_HK
dc.subjectIn-line-
dc.titleThe discovery based on GLIMPSE data of a protostar driving a bipolar outflowen_HK
dc.typeArticleen_HK
dc.identifier.emailYuan, J: jhyuan@nao.cas.cnen_HK
dc.identifier.emailHsia, C: xiazh@hku.hk-
dc.identifier.authorityHsia, CH=rp00706en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1051/0004-6361/201117858en_HK
dc.identifier.scopuseid_2-s2.0-84859313624en_HK
dc.identifier.hkuros209211en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-84859313624&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume540, article no. A95en_HK
dc.identifier.isiWOS:000303315400109-
dc.publisher.placeFranceen_HK
dc.identifier.scopusauthoridMiao, J=55171680800en_HK
dc.identifier.scopusauthoridHsia, CH=14058287100en_HK
dc.identifier.scopusauthoridHuang, YF=55169104400en_HK
dc.identifier.scopusauthoridLi, JZ=55171212200en_HK
dc.identifier.scopusauthoridYuan, JH=55170380200en_HK
dc.identifier.issnl0004-6361-

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