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

70 citations · 177 across the 9 of their papers we have counts for

collaborators

6 papers

astro-ph.SR202332 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.SR202370 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.SR20238 cited

Evolution of the outflow in the water fountain source IRAS 180432116

L. Uscanga, H. Imai, J. F. Gómez +5

We present the spectral and spatial evolution of HO masers associated with the water fountain source IRAS 180432116 found in the observations with the Nobeyama 45 m telescop…

astro-ph.SR202318 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.GA20235 cited

Very long baseline interferometry observations of the high-redshift blazar candidate J0141-5427

K. É. Gabányi, S. Belladitta, S. Frey +7

Active galactic nuclei (AGN) have been observed as far as redshift z~7. They are crucial in investigating the early Universe as well as the growth of supermassive black holes at th…

astro-ph.IM201644 cited

MultiView High Precision VLBI Astrometry at Low Frequencies

Maria J. Rioja, Richard Dodson, Gabor Orosz +2

The arrival of the Square Kilometer Array (SKA) will revitalise all aspects of Very Long Baseline Interferometry (VLBI) astronomy at the lower frequencies. In the last decade there…