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Authordc.contributor.authorJhan, Kai-Syun
Authordc.contributor.authorLee, Chin-Fei
Authordc.contributor.authorJohnstone, Doug
Authordc.contributor.authorLiu, Tie
Authordc.contributor.authorLiu, Sheng-Yuan
Authordc.contributor.authorHirano, Naomi
Authordc.contributor.authorTatematsu, Ken'ichi
Authordc.contributor.authorDutta, Somnath
Authordc.contributor.authorMoraghan, Anthony
Authordc.contributor.authorShang, Hsein
Authordc.contributor.authorLee, Jeong-Eun
Authordc.contributor.authorLi, Shanghuo
Authordc.contributor.authorLiu, Chun-Fan
Authordc.contributor.authorHsu, Shih-Ying
Authordc.contributor.authorKwon, Woojin
Authordc.contributor.authorSahu, Dipen
Authordc.contributor.authorLiu, Xun-Chuan
Authordc.contributor.authorKim, Kee-Tae
Authordc.contributor.authorLuo, Qiuyi
Authordc.contributor.authorQin, Sheng-Li
Authordc.contributor.authorSanhueza, Patricio
Authordc.contributor.authorBronfman Aguiló, Leonardo Jaime
Authordc.contributor.authorQizhou, Zhang
Authordc.contributor.authorEden, David
Authordc.contributor.authorTraficante, Alessio
Authordc.contributor.authorLee, Chang Won
Cita de ítemdc.identifier.citationThe Astrophysical Journal Letters, 931:L5 (9pp), 2022es_ES
Abstractdc.description.abstractWe have selected six sources (G209.55-19.68S2, G205.46-14.56S1(-)A, G203.21-11.20W2, G191.90-11.21S, G205.46-14.56S3, and G206.93-16.61W2) from the Atacama Large Millimeter/submillimeter Array Survey of Orion Planck Galactic Cold Clumps (ALMASOP), in which these sources have been mapped in the CO (J = 2-1), SiO (J = 5-4), and (CO)-O-18 (J = 2-1) lines. These sources have high-velocity SiO jets surrounded by low-velocity CO outflows. The SiO jets consist of a chain of knots. These knots have been thought to be produced by semiperiodic variations in jet velocity. Therefore, we adopt a shock-forming model, which uses such variations to estimate the inclination angle and velocity of the jets. We also derive the inclination angle of the CO outflows using the wide-angle wind-driven shell model and find it to be broadly consistent with that of the associated SiO jets. In addition, we apply this shock-forming model to another three protostellar sources with SiO jets in the literature-HH 211, HH 212, and L1448C(N)-and find that their inclination angle and jet velocity are consistent with those previously estimated from proper-motion and radial-velocity studies.es_ES
Patrocinadordc.description.sponsorshipMinistry of Science and Technology, Taiwan MoST 107-2119-M-001-040-MY3 110-2112-M-001-021-MY3 Academia Sinica - Taiwan AS-IA-108-M01 National Research Foundation of Korea NRF- 2019R1A2C1010851 NRC Canada Natural Sciences and Engineering Research Council of Canada (NSERC) MoST 109-2112-M-001-023 109-2112-M-001-048 National Research Foundation of Korea Ministry of Science, ICT & Future Planning, Republic of Korea Ministry of Science & ICT (MSIT), Republic of Korea 2021R1A2C1011718 Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science 18H01259 ANID BASAL ACE210002 FB210003 National Natural Science Foundation of China (NSFC) 12033005 12073061 12122307 Chinese Academy of Sciences 114231KYSB20200009 Shanghai Pujiang Program 20PJ1415500 China Manned Space Project CMS-CSST-2021-B06 European Research Council (ERC) 855130 Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research (KAKENHI) 20H05645 Ministry of Science and Technology, Taiwan 109-2112-M-001-028- 110-2112-M-001-019-es_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 United States*
Link to Licensedc.rights.uri*
Sourcedc.sourceThe Astrophysical Journal Letterses_ES
Keywordsdc.subjectSubmillimeter array observationses_ES
Keywordsdc.subjectNumerical simulationses_ES
Keywordsdc.subjectTransient surveyes_ES
Títulodc.titleALMA survey of Orion planck galactic cold clumps (ALMASOP): deriving inclination angle and velocity of the protostellar jets from their SiO knotses_ES
Document typedc.typeArtículo de revistaes_ES
dc.description.versiondc.description.versionVersión publicada - versión final del editores_ES
dcterms.accessRightsdcterms.accessRightsAcceso abiertoes_ES
Indexationuchile.indexArtículo de publícación WoSes_ES

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