Multi-scale view of star formation in IRAS 21078+5211: From clump fragmentation to disk wind
arXiv:2102.04872 · doi:10.1051/0004-6361/202039837
Abstract
In the massive star-forming region IRAS 21078+5211, a highly fragmented cluster (0.1~pc in size) of molecular cores is observed, located at the density peak of an elongated (1~pc in size) molecular cloud. A small (1~km/s per 0.1~pc) LSR velocity (Vlsr) gradient is detected across the axis of the molecular cloud. Assuming we are observing a mass flow from the harboring cloud to the cluster, we derive a mass infall rate of about 10^{-4}~M_{sun}~yr^{-1}. The most massive cores (labeled 1, 2, and 3) are found at the center of the cluster, and these are the only ones that present a signature of protostellar activity in terms of emission from high-excitation molecular lines or a molecular outflow. We reveal an extended (size about 0.1~pc), bipolar collimated molecular outflow emerging from core 1. We believe this is powered by a (previously discovered) compact (size <= 1000~au) radio jet, ejected by a YSO embedded in core 1 (named YSO-1), since the molecular outflow and the radio jet are almost parallel and have a comparable momentum rate. By means of high-excitation lines, we find a large (14~km/s over 500~au) Vlsr gradient at the position of YSO-1, oriented approximately perpendicular to the radio jet. Assuming this is an edge-on, rotating disk and fitting a Keplerian rotation pattern, we determine the YSO-1 mass to be 5.6+/-2.0~M_{sun}. The water masers (previously observed with VLBI) emerge within 100-300~au from YSO-1 and are unique tracers of the jet kinematics. Their three-dimensional (3D) velocity pattern reveals that the gas flows along, and rotates about, the jet axis. We show that the 3D maser velocities are fully consistent with the magneto-centrifugal disk-wind models predicting a cylindrical rotating jet. Under this hypothesis, we determine the jet radius to be about 16~au and the corresponding launching radius and terminal velocity to be about 2.2~au and 200~km/s, respectively.
arXiv comment25 pages, 16 figures
References in corpus (56)
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- Trigonometric Parallaxes of High Mass Star Forming Regions: the Structure and Kinematics of the Milky Way
- The Formation of Massive Stars from Turbulent Cores
- Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way
- Hi-GAL: the Herschel infrared Galactic Plane Survey
- Filamentary structure of star-forming complexes
- The SCUBA Legacy Catalogue: Continuum Objects Detected by SCUBA
- Massive star formation: Nurture, not nature
- Global Hierarchical Collapse In Molecular Clouds. Towards a Comprehensive Scenario
- The Red MSX Source Survey: the Massive Young Stellar Population of our Galaxy
- HST/STIS Spectroscopy of the Optical Outflow from DG Tau: Indications for Rotation in the Initial Jet Channel
- Hierarchical fragmentation and differential star formation in the Galactic "Snake": infrared dark cloud G11.11-0.12
- Inefficient star formation through turbulence, magnetic fields and feedback
- The ALMA Survey of 70 m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation
- ON the Nature of the Local Spiral Arm of the Milky Way
- Rotation of Jets from Young Stars: New Clues from the Hubble Space Telescope Imaging Spectrograph
- Trigonometric Parallaxes of Massive Star Forming Regions: I. S 252 & G232.6+1.0
- The Origin of Massive Stars: The Inertial-Inflow Model
- The RMS Survey: Critical Tests of Accretion Models for the Formation of Massive Stars
- A distance limited sample of massive molecular outflows
- Partition functions and equilibrium constants for diatomic molecules and atoms of astrophysical interest
- Radio Jets from Young Stellar Objects
- eXtended CASA Line Analysis Software Suite (XCLASS)
- Precession of collimated outflows from young stellar objects
- Dynamics of cluster-forming hub-filament systems: The case of the high-mass star-forming complex Monoceros R2
- Filamentary Fragmentation and Accretion in High-Mass Star-Forming Molecular Clouds
- Filamentary Accretion Flows in the Infrared Dark Cloud G14.225-0.506 Revealed by ALMA
- The Role of Magnetic Fields in Protostellar Outflows and Star Formation
- Complex Structure in Class 0 Protostellar Envelopes III: Velocity Gradients in Non-Axisymmetric Envelopes, Infall or Rotation?
- A Multi-Epoch Study of the Radio Continuum Emission of Orion Source I: Constraints on the Disk Evolution of a Massive YSO and the Dynamical History of Orion BN/KL
- ALMA survey of massive cluster progenitors from ATLASGAL. Limited fragmentation at the early evolutionary stage of massive clumps
- The jet and the disk of the HH 212 low-mass protostar imaged by ALMA: SO and SO2 emission
- Line Profiles of Cores within Clusters: II Signatures of Dynamical Collapse during High Mass Star Formation
- Jets and outflows of massive protostars - From cloud collapse to jet launching and cloud dispersal
- The Physical and chemical structure of Sagittarius B2 -- IV. Converging filaments in the high-mass cluster forming region Sgr B2(N)
- Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core
- Core fragmentation and Toomre stability analysis of W3(H2O): A case study of the IRAM NOEMA large program CORE
- Very Large Array Observations of Ammonia in Infrared-Dark Clouds II: Internal Kinematics
- Evidence of a past disc-disc encounter: HV and DO Tau
- A `Water Spout' Maser Jet in S235AB-MIR
- Misalignment of Magnetic Fields, Outflows and Discs in Star-forming Clouds
- Does misalignment between magnetic field and angular momentum enhance or suppress circumstellar disk formation?
- Protostellar Outflows at the EarliesT Stages (POETS). I. Radio thermal jets at high resolution nearby HO maser sources
- The density structure of the L1157 molecular outflow
- Protostellar Outflows at the EarliesT Stages (POETS). II. A possible radio synchrotron jet associated with the EGO G035.02+0.35
- Origin of Misalignments: Protostellar Jet, Outflow, Circumstellar Disc, and Magnetic Field
- Fragmentation and disk formation during high-mass star formation: The IRAM NOEMA (Northern Extended Millimeter Array) large program CORE
- HST-Scale 3D simulations of MHD disc winds : A rotating two-component jet structure
- How first hydrostatic cores, tidal forces and gravo-turbulent fluctuations set the characteristic mass of stars
- Protostellar Outflows at the EarliesT Stages (POETS). III. H2O masers tracing disk-winds and jets near luminous YSOs
- IRAS23385+6053: An embedded massive cluster in the making
- Fragmentation, rotation and outflows in the high-mass star-forming region IRAS 23033+5951. A case study of the IRAM NOEMA large program CORE
- Disk wind feedback from high-mass protostars
- Protostellar Outflows at the EarliesT Stages (POETS). IV. Statistical properties of the 22 GHz H2O masers
- The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"
- ALMA observations of two massive and dense MALT90 clumps
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- Snapshot of a magnetohydrodynamic disk wind traced by water maser observations
- Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution -- Insights from the IRAM NOEMA large program CORE
- Modeling disks and magnetic outflows around a forming massive star: I. Investigating the two layer-structure of the accretion disk
- Modeling disks and magnetic outflows around a forming massive star: II. Dynamics of jets from massive protostars
- Detection of a new molecular cloud in the LHAASO J2108+5157 region supporting a hadronic PeVatron scenario
- The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"
- The Role of Thermal Instability in Accretion Outbursts in High-Mass Stars
- ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clump
- Protostellar Outflows at the EarliesT Stages (POETS) V. The launching mechanism of protostellar winds via water masers
- The magnetic field of a magnetohydrodynamic disk wind: Water maser observations and simulations
- Looking for evidence of high-mass star formation at core scale in a massive molecular clump
- Episodic accretion in high-mass star formation: An analysis of thermal instability for axially symmetric disks
- Revisiting G29.862-0.0044: a jet cavity disrupted by an outflow in a likely young stellar object wide binary system
- Unveiling the substructure of the massive clump AGAL G035.133000.7450
- Are Kronberger 80 and/or Kronberger 82 regions PeVatron candidates for LHAASO J2108+5157?
- ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- V. Hierarchical fragmentation and gas dynamics in IRDC G034.43+00.24