activity
20142026
most citedFOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results

205 citations · 1.8k across the 99 of their papers we have counts for

collaborators

100 papers

astro-ph.GA2026

ALMA Observations of Molecular Complexity in the Large Magellanic Cloud: The N83 Star-Forming Region

Marta Sewiło, Amanda Broadmeadow, Roya Hamedani Golshan +9

We report the results of the 1.2 mm continuum and molecular line 0.1 parsec-scale observations with the Atacama Large Millimeter/submillimeter Array of two fields in the star…

astro-ph.HE2026

ALMA Observations of DEM L241/LMC P3 in the Large Magellanic Cloud: Evidence for the Formation of Cool Molecular Jets Driven by a Microquasar

Yasuo Fukui, Bhuvana G. R., Hidetoshi Sano +17

We present ALMA observations of DEML 241/LMC P3, the most luminous -ray binary consisting of a compact object and an O star, in CO emission. We have found an one-sided jet-like…

astro-ph.HE2026

Molecular and Atomic Gas Associated with the Gamma Ray Supernova Remnant RCW 103

H. Inoue, Y. Asano, R. G. Bhuvana +15

We present a study of the interstellar molecular and atomic gas associated with the gamma-ray supernova remnant (SNR) RCW 103 using the Mopra CO( = 1-0), Atacama Large Mi…

astro-ph.GA2026

From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system

Jihye Hwang, Doris Arzoumanian, Yoshito Shimajiri +5

Hub-filament systems (HFSs) play an important role in the formation of massive stars and star clusters. Although the velocity structures along dense filaments have been studied, th…

astro-ph.GA2026

An AGN in the Antennae galaxies ?

Shinya Komugi, Toshiki Saito, Tomonari Michiyama +5

Time variability is a strong probe of energetic phenomena which occur at small spatial scales, like Active Galactic Nuclei (AGN). We use ALMA observations at 100 GHz executed over…

astro-ph.GA2026

Observations of DNC and DCO toward the -shaped Filament and Starless Cores in the Orion Molecular Clouds

Ken'ichi Tatematsu, Atsushi Nishimura, Hideo Ogawa +25

Although the deuterium fraction is known to be a powerful evolutionary tracer, its variation within individual molecular cloud cores is still poorly understood. The northern …