activity
20172026
most citedFOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results

205 citations · 422 across the 18 of their papers we have counts for

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Showing astro-ph.GAShow all

30 papers · 1 filter

astro-ph.GA2026

The trigonometric parallax of IRAS 23385+6053 and physical properties of molecular clouds based on the VLBI astrometry

Shota Hamada, Mikito Kohno, Toshihiro Omodaka +5

We performed very long baseline interferometry (VLBI) observations to measure the trigonometric parallax of HO maser sources in the outer massive star-forming region IRAS 23385…

astro-ph.GA2025

Head-tail molecular clouds falling onto the Milky Way disk

Mikito Kohno, Yasuo Fukui, Takahiro Hayakawa +13

We report discovery of two CO clouds which are likely falling down to the Galactic plane at more than km s. The clouds show head-tail distributions elongated perpendicu…

astro-ph.GA2025

The inner rotation curve of the Milky Way

Y. Sofue, M. Kohno

We derived the inner rotation curve (RC) of the Milky Way by applying the terminal velocity method (TVM) to the longitude-velocity diagrams (LVD) made from the large-scale survey d…

astro-ph.GA2025

A catalog of molecular clouds possibly associated with Galactic infrared bubbles I. The Southern Galactic plane

Mikito Kohno, Yoshiaki Sofue, Yasuo Fukui +1

We have carried out a morphological search for molecular clouds possibly associated with 48 Galactic infrared bubbles with angular radii of in the southern Galactic plane of…

astro-ph.GA2024

The CO-to-H Conversion Factor in the Central Molecular Zone of the Milky Way using CO isotopologues

Mikito Kohno, Yoshiaki Sofue

We performed correlation analyses between the CO and CO 1-0 line intensities in order to derive the variability of the CO-to-H conversion factor ($X_{\rm CO,…

astro-ph.GA2023

The CO-to-H Conversion Factor of Galactic Giant Molecular Clouds using CO isotopologues: High-resolution maps

Mikito Kohno, Yoshiaki Sofue

We investigated the correlation between intensities of the CO and CO (-0) lines toward the Galactic giant molecular clouds (GMCs) W51A, W33, N35-N36 complex, W49…