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20102026
most citedResolved images of a protostellar outflow launched by an extended disk wind

167 citations · 699 across the 21 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

A Search for Dust in the Outflow of the HH212 Class 0 Protostellar System

Adele L. Plunkett, Per Bjerkeli, Jon P. Ramsey +2

Perhaps the most visually striking phenomenon during star formation is the ejection of material along the direction of the protostar's rotational axis. Observed in the form of mole…

astro-ph.SR2024★ 15 cited

The Asymmetric Bipolar Fe II Jet and H2 Outflow of TMC1A Resolved with JWST's NIRSpec IFU

Korash Assani, Daniel Harsono, Jon Ramsey +10

(abridged) Protostellar outflows exhibit large variations in their structure depending on the observed gas emission. This study analyzes the atomic jet and molecular outflow in the…

astro-ph.SR2023★ 34 cited

JWST Peers into the Class I Protostar TMC1A: Atomic Jet and Spatially Resolved Dissociative Shock Region

Daniel Harsono, Per Bjerkeli, Jon Ramsey +6

Outflows and winds launched from young stars play a crucial role in the evolution of protostars and the early stages of planet formation. However, the specific details of the mecha…

astro-ph.SR2019★ 47 cited

Kinematics around the B335 protostar down to au scales

Per Bjerkeli, Jon P. Ramsey, Daniel Harsono +6

Context. The relationship between outflow launching and formation of accretion disks around young stellar objects is still not entirely understood, which is why spectrally and spat…

astro-ph.SR2019★ 14 cited

MHD simulations of the formation and propagation of protostellar jets to observational length scales

Jon P. Ramsey, David A. Clarke

We present 2.5-D global, ideal MHD simulations of magnetically and rotationally driven protostellar jets from Keplerian accretion discs, wherein only the initial magnetic field str…

astro-ph.SR2018★ 100 cited

Evidence for the start of planet formation in a young circumstellar disk

Daniel Harsono, Per Bjerkeli, Matthijs H. D. van der Wiel +4

The growth of dust grains in protoplanetary disks is a necessary first step towards planet formation. This growth has been inferred via observations of thermal dust emission toward…