activity
20172022
most citedMillimetre-wave Emission from an Intermediate-Mass Black Hole Candidate in the Milky Way

51 citations · 159 across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.GA20225 cited

Catalog of High Velocity Dispersion Compact Clouds in the Central Molecular Zone of Our Galaxy

Tomoharu Oka, Asaka Uruno, Rei Enokiya +5

This study developed an automated identification procedure for compact clouds with broad velocity widths in the spectral line data cubes of highly crowded regions. The procedure wa…

astro-ph.GA20213 cited

Broad-velocity-width Molecular Features in the Galactic Plane

Hiroki Yokozuka, Tomoharu Oka, Shunya Takekawa +2

We performed a systematic search for broad-velocity-width molecular features (BVFs) in the disk part of our Galaxy by using the CO J = 1-0 survey data obtained with the Nobeyama Ra…

astro-ph.GA20217 cited

New Look at the Molecular Superbubble Candidate in the Galactic Center

Shiho Tsujimoto, Tomoharu Oka, Shunya Takekawa +10

The region in the Galactic center is characterized by multiple shell-like structures and their extremely broad velocity widths. We revisit the molecular supe…

astro-ph.HE2020

Time Variations in the Flux Density of Sgr A* at 230 GHz Detected with ALMA

Yuhei Iwata, Tomoharu Oka, Masato Tsuboi +2

A radio source at the Galactic center Sgr A* is a prime supermassive black hole candidate and therefore key to developing our understanding of them. Time variations in the 230 GHz…

astro-ph.GA202030 cited

The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center

Shunya Takekawa, Tomoharu Oka, Yuhei Iwata +2

We report the results of high-resolution molecular line observations of the high-velocity compact cloud HCN-0.085-0.094 with the Atacama Large Millimeter/submillimeter Array. The H…

astro-ph.GA2019

An energetic high-velocity compact cloud: CO0.31+0.11

Shunya Takekawa, Tomoharu Oka, Sekito Tokuyama +5

We have discovered an energetic high-velocity compact cloud CO0.31+0.11 in the central molecular zone of our Galaxy. CO0.31+0.11 is located at a projected distance of $\sim 4…