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19932026
most citedUnified Rotation Curve of the Galaxy -- Decomposition into de Vaucouleurs Bulge, Disk, Dark Halo, and the 9-kpc Rotation Dip --

314 citations · 652 across the 17 of their papers we have counts for

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astro-ph2008★ 314 cited

Unified Rotation Curve of the Galaxy -- Decomposition into de Vaucouleurs Bulge, Disk, Dark Halo, and the 9-kpc Rotation Dip --

Y. Sofue, M. Honma, T. Omodaka

We present a unified rotation curve of the Galaxy re-constructed from the existing data by re-calculating the distances and velocities for a set of galactic constants R_0=8 kpc and…

astro-ph2003★ 49 cited

The Virgo High-Resolution CO Survey I. CO Atlas

Y. Sofue, J. Koda, H. Nakanishi +4

We present the results of the Virgo high-resolution CO survey (ViCS) obtained with the Nobeyama Millimeter-wave Array (NMA). This survey was made in the course of a long-term proje…

astro-ph2001★ 13 cited

Hubble Constant at Intermediate Redshift using the CO-Line Tully-Fisher Relation

Y. Tutui, Y. Sofue, M. Honma +2

We have determined distances and Hubble ratios for galaxies at intermediate redshifts, cz=about 10,000 to 35,000 km/s, by applying the CO-line Tully-Fisher relation to our 12CO (J=…

astro-ph1999★ 249 cited

Central Rotation Curves of Spiral Galaxies

Y. Sofue, Y. Tutui, M. Honma +4

We present high-resolution central-to-outer rotation curves for Sb, SBb, Sc, and SBc galaxies. We discuss their general characteristics, particularly their central behavior, as wel…

astro-ph1996★ 7 cited

Distance Measurement of Galaxies to Redshift of 0.1 using the CO-Line Tully-Fisher Relation

Y. Sofue, F. Schoeniger, M. Honma +5

We report on the first results of a long-term project to derive distances of galaxies at cosmological distances by applying the CO-line width-luminosity relation. We have obtained…

astro-ph1993★ 20 cited

A Polar-Nulceus Dark Lane in the Barred Spiral M83: Three-Dimensional Accretion in the Nucleus

Y. Sofue, K. Wakamatsu

The central region of the barred spiral galaxy M83 reveals a polar-nucleus dust lane, wh ich extends from the NE molecular bar and crosses the central bulge. Its SW counterpart is…