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ALMA and VLBA views on the outflow associated with an O-type protostar in G26.50+0.28
Wu, Gang1,2; Henkel, Christian1,2,3; Xu, Ye4; Brunthaler, Andreas1; Menten, Karl M.1; Qiu, Keping5; Li, Jingjing4; Zhang, Bo6; Esimbek, Jarken2
2023-09-08
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume677Pages:A80
Contribution Rank2
AbstractProtostellar jets and outflows are essential ingredients of the star formation process. A better understanding of this phenomenon is important in its own right as well as for many fundamental aspects of star formation. Jets and outflows associated with O-type protostars are rarely studied with observations reaching the close vicinity of the protostars. In this work, we report high-resolution ALMA and VLBA observations to reveal a clear and consistent picture of an outflow associated with an O-type protostar candidate in the G26.50+0.28 region. These observations reveal, for the first time, a collimated jet located in the middle of the outflow cavity. The jet is found to be perpendicular to an elongated disk/toroid and its velocity gradient. The collimated jet appears to show a small amplitude (a & AP;0 & DEG;.06) counterclockwise precession, when looking along the blueshifted jet axis from the strongest continuum source MM1, with a precession length of 0.22 pc. The inclination of the jet is likely to be very low (& AP;8 & DEG;), which makes it a promising target to study its transverse morphologies and kinematics. However, no clear evidence of jet rotation is found in the ALMA and VLBA observations. The three-dimensional velocities of the water maser spots appear to show the same absolute speed with respect to different opening angles, suggesting the jet winds may be launched in a relatively small region. This favors the X-wind model, that is, jets are launched in a small area near the inner disk edge.
KeywordISM: jets and outflows stars: formation masers radio lines: ISM
DOI10.1051/0004-6361/202345893
Indexed BySCI
Language英语
WOS KeywordMOLECULAR OUTFLOWS ; ACCRETION DISKS ; JET ; STAR ; VELOCITY ; COLLIMATION ; PARALLAXES ; DRIVEN ; MASER ; AU
Funding ProjectNational Key R&D Program of China[2022YFA1603103] ; CAS Light ofWest China Program[2021-XBQNXZ-028] ; National Natural Science foundation of China[12103082] ; National Natural Science foundation of China[11603063] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2022D01A362] ; Youth Innovation Promotion Association CAS
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001065619100002
PublisherEDP SCIENCES S A
Funding OrganizationNational Key R&D Program of China ; CAS Light ofWest China Program ; National Natural Science foundation of China ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; Youth Innovation Promotion Association CAS
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5514
Collection射电天文研究室_恒星形成与演化研究团组
Corresponding AuthorWu, Gang
Affiliation1.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
2.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
3.King Abdulaziz Univ, Astron Dept, POB 80203, Jeddah 21589, Saudi Arabia
4.Chinese Acad Sci, Purple Mt Observ, 8 Yuanhua Rd, Nanjing 210034, Peoples R China
5.Nanjing Univ, Sch Astron & Space Sci, 163 Xianlin Ave, Nanjing 210023, Peoples R China
6.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wu, Gang,Henkel, Christian,Xu, Ye,et al. ALMA and VLBA views on the outflow associated with an O-type protostar in G26.50+0.28[J]. ASTRONOMY & ASTROPHYSICS,2023,677:A80.
APA Wu, Gang.,Henkel, Christian.,Xu, Ye.,Brunthaler, Andreas.,Menten, Karl M..,...&Esimbek, Jarken.(2023).ALMA and VLBA views on the outflow associated with an O-type protostar in G26.50+0.28.ASTRONOMY & ASTROPHYSICS,677,A80.
MLA Wu, Gang,et al."ALMA and VLBA views on the outflow associated with an O-type protostar in G26.50+0.28".ASTRONOMY & ASTROPHYSICS 677(2023):A80.
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