activity
19992026
most citedRadio Continuum and Recombination Line Study of UC HII Regions with Extended Envelopes

136 citations · 3.2k across the 138 of their papers we have counts for

collaborators
Showing 2023Show all

8 papers · 1 filter

astro-ph.SR2023

The Limits of Water Maser Kinematics: Insights from High-Mass Protostar AFGL 5142-MM1

Zulfazli Rosli, Ross A. Burns, Affan Adly Nazri +14

Multi-epoch VLBI observations measure 3D water maser motions in protostellar outflows, enabling analysis of inclination and velocity. However, these analyses assume that water mase…

astro-ph.GA2023

The ALMA-QUARKS survey: -- I. Survey description and data reduction

Xunchuan Liu, Tie Liu, Lei Zhu +31

This paper presents an overview of the QUARKS survey, which stands for `Querying Underlying mechanisms of massive star formation with ALMA-Resolved gas Kinematics and Structures'.…

astro-ph.GA2023★ 1 cited

Neutral atomic and molecular clouds and star formation in the outer Carina arm

Geumsook Park, Bon-Chul Koo, Kee-Tae Kim +1

We present a comprehensive investigation of HI (super)clouds, molecular clouds (MCs), and star formation in the Carina spiral arm of the outer Galaxy. Utilizing HI4PI and CfA CO su…

astro-ph.GA2023★ 1 cited

Episodic Accretion in Protostars -- An ALMA Survey of Molecular Jets in the Orion Molecular Cloud

Somnath Dutta, Chin-Fei Lee, Doug Johnstone +20

Protostellar outflows and jets are almost ubiquitous characteristics during the mass accretion phase, and encode the history of stellar accretion, complex-organic molecule (COM) fo…

astro-ph.SR2023★ 32 cited

A Keplerian disk with a four-arm spiral birthing an episodically accreting high-mass protostar

R. A. Burns, Y. Uno, N. Sakai +34

High-mass protostars (M 8 M) are thought to gain the majority of their mass via short, intense bursts of growth. This episodic accretion is thought to be faci…

astro-ph.SR2023★ 70 cited

A heat-wave of accretion energy traced by masers in the G358-MM1 high-mass protostar

R. A. Burns, K. Sugiyama, T. Hirota +20

High-mass stars are thought to accumulate much of their mass via short, infrequent bursts of disk-aided accretion. Such accretion events are rare and difficult to observe directly…