activity
20142026
most citedDisk-Driven Rotating Bipolar Outflow in Orion Source I

144 citations · 867 across the 39 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

25 papers · 1 filter

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…

astro-ph.SR2023★ 18 cited

Multi-frequency VLBI observations of maser lines during the 6.7~GHz maser flare in the high-mass young stellar object G24.330.14}

A. Kobak, A. Bartkiewicz, M. Szymczak +13

Recent studies have shown that 6.7 GHz methanol maser flares can be a powerful tool for verifying the mechanisms of maser production and even the specific signatures of accretion r…

astro-ph.SR2021★ 1 cited

Infrared observations of the flaring maser source G358.93-0.03 -- SOFIA confirms an accretion burst from a massive young stellar object

B. Stecklum, V. Wolf, H. Linz +24

Class II methanol masers are signs of massive young stellar objects (MYSOs). Recent findings show that MYSO accretion bursts cause flares of these masers. Thus, maser monitoring ca…

astro-ph.SR2020★ 10 cited

FLASHING: New high-velocity HO masers in IRAS 182860959

Hiroshi Imai, Yuri Uno, Daichi Maeyama +8

We discovered new high-velocity components of HO maser emission in one of the "water fountain" sources, IRAS~182860959, which has been monitored using the Nobeyama 45 m tele…

astro-ph.SR2020★ 12 cited

Magnetic Field Structure of Orion Source I

Tomoya Hirota, Richard L. Plambeck, Melvyn C. H. Wright +6

We observed polarization of the SiO rotational transitions from Orion Source I (SrcI) to probe the magnetic field in bipolar outflows from this high mass protostar. Both 43 GHz …