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dc.contributorGraduate Institute of Astronomy and Astrophysics, National Taiwan University, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan; Academia Sinica Institute of Astronomy and Astrophysics, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan
dc.contributorAcademia Sinica Institute of Astronomy and Astrophysics, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan; Graduate Institute of Astronomy and Astrophysics, National Taiwan University, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan
dc.contributorNational Research Council of Canada, Herzberg, Astronomy and Astrophysics Research Centre, 5071 West Saanich Road, V9E 2E7 Victoria (BC), Canada; Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 5C2, Canada
dc.contributorShanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, People's Republic of China
dc.contributorAcademia Sinica Institute of Astronomy and Astrophysics, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan
dc.contributorNobeyama Radio Observatory, National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 462-2 Nobeyama, Minamimaki, Minamisaku, Nagano 384-1305, Japan; Department of Astronomical Science, SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
dc.contributorSchool of Space Research, Kyung Hee University, Yongin-Si, Gyeonggi-Do 17104, Republic of Korea
dc.contributorKorea Astronomy and Space Science Institute (KASI), 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea
dc.contributorAcademia Sinica Institute of Astronomy and Astrophysics, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan; Graduate Institute of Physics, National Taiwan University, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan
dc.contributorDepartment of Earth Science Education, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea; SNU Astronomy Research Center, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea
dc.contributorKorea Astronomy and Space Science Institute (KASI), 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea; University of Science and Technology, Korea (UST), 217 Gajeong-ro, Yuseong-gu, Daejeon 34113, Republic of Korea
dc.contributorDepartment of Astronomy, Yunnan University, and Key Laboratory of Particle Astrophysics of Yunnan Province, Kunming, 650091, People's Republic of China
dc.contributorDepartment of Astronomical Science, SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
dc.contributorDepartamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile
dc.contributorCenter for Astrophysics-Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
dc.contributorArmagh Observatory and Planetarium, College Hill, Armagh, BT61 9DB, UK
dc.contributorIAPS-INAF, via Fosso del Cavaliere 100, I-00133, Rome, Italy
dc.contributor-
dc.contributor.authorJhan, Kai-Syun
dc.contributor.authorLee, Chin-Fei
dc.contributor.authorJohnstone, Doug
dc.contributor.authorLiu, Tie
dc.contributor.authorLiu, Sheng-Yuan
dc.contributor.authorHirano, Naomi
dc.contributor.authorTatematsu, Ken'ichi
dc.contributor.authorDutta, Somnath
dc.contributor.authorMoraghan, Anthony
dc.contributor.authorShang, Hsien
dc.contributor.authorLee, Jeong-Eun
dc.contributor.authorLi, Shanghuo
dc.contributor.authorLiu, Chun-Fan
dc.contributor.authorHsu, Shih-Ying
dc.contributor.authorKwon, Woojin
dc.contributor.authorSahu, Dipen
dc.contributor.authorLiu, Xun-Chuan
dc.contributor.authorKim, Kee-Tae
dc.contributor.authorLuo, Qiuyi
dc.contributor.authorQin, Sheng-Li
dc.contributor.authorSanhueza, Patricio
dc.contributor.authorBronfman, Leonardo
dc.contributor.authorQizhou, Zhang
dc.contributor.authorEden, David
dc.contributor.authorTraficante, Alessio
dc.contributor.authorLee, Chang Won
dc.contributor.authorAlmasop Team
dc.date.accessioned2024-02-01T17:11:19Z
dc.date.available2024-02-01T17:11:19Z
dc.date.issued2022-05-01T00:00:00Z
dc.identifier.doi10.3847/2041-8213/ac6a53
dc.identifier.doi10.48550/arXiv.2204.12731
dc.identifier.other2022arXiv220412731J
dc.identifier.otherastro-ph.GA
dc.identifier.otherastro-ph.SR
dc.identifier.other10.48550/arXiv.2204.12731
dc.identifier.otherarXiv:2204.12731
dc.identifier.other10.3847/2041-8213/ac6a53
dc.identifier.other2022ApJ...931L...5J
dc.identifier.other2022arXiv220412731J
dc.identifier.other0000-0003-2069-1403
dc.identifier.other0000-0002-3024-5864
dc.identifier.other0000-0002-6773-459X
dc.identifier.other0000-0002-5286-2564
dc.identifier.other0000-0003-4603-7119
dc.identifier.other0000-0001-9304-7884
dc.identifier.other0000-0002-8149-8546
dc.identifier.other0000-0002-2338-4583
dc.identifier.other-
dc.identifier.other0000-0001-8385-9838
dc.identifier.other0000-0003-3119-2087
dc.identifier.other0000-0003-1275-5251
dc.identifier.other0000-0002-1624-6545
dc.identifier.other0000-0002-1369-1563
dc.identifier.other0000-0003-4022-4132
dc.identifier.other0000-0002-4393-3463
dc.identifier.other0000-0003-2412-7092
dc.identifier.other0000-0003-2302-0613
dc.identifier.other0000-0002-7125-7685
dc.identifier.other0000-0002-9574-8454
dc.identifier.other0000-0003-2384-6589
dc.identifier.other0000-0002-5881-3229
dc.identifier.other0000-0003-1665-6402
dc.identifier.other0000-0002-3179-6334
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1400
dc.description.abstractWe have selected six sources (G209.55-19.68S2, G205.46-14.56S1<SUB>-</SUB>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 C<SUP>18</SUP>O (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.
dc.publisherThe Astrophysical Journal
dc.titleALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Deriving Inclination Angle and Velocity of the Protostellar Jets from Their SiO Knots
dc.typearticle
dc.source.journalApJL
dc.source.journalApJL..931
dc.source.volume931
refterms.dateFOA2024-02-01T17:11:19Z
dc.identifier.bibcode2022ApJ...931L...5J


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