activity
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

collaborators

22 papers

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.EP2023

Deep Search For Molecular Oxygen in TW Hya

Becky J. Williams, L. Ilsedore Cleeves, Christian Eistrup +1

The dominant form of oxygen in cold molecular clouds is gas-phase carbon monoxide (CO) and ice-phase water (HO). Yet, in planet-forming disks around young stars, gas-phase CO a…

astro-ph.GA2023★ 8 cited

Episodic infall towards a compact disk in B335?

Per Bjerkeli, Jon P. Ramsey, Daniel Harsono +7

Previous observations of B335 have presented evidence of ongoing infall in various molecular lines, e.g., HCO, HCN, CO. There have been no confirmed observations of a rotationa…

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.GA2023★ 5 cited

Disk Wind Feedback from High-mass Protostars. II. The Evolutionary Sequence

Jan E. Staff, Kei E. I. Tanaka, Jon P. Ramsey +2

Star formation is ubiquitously associated with the ejection of accretion-powered outflows that carve bipolar cavities through the infalling envelope. This feedback is expected to b…