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20042023
most citedFirst Results from High Angular Resolution ALMA Observations Toward the HL Tau Region

1.2k citations · 2.9k across the 43 of their papers we have counts for

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astro-ph2008★ 2 cited

Tracing star formation in galaxies with molecular line and continuum observations

K. Kohno, K. Muraoka, B. Hatsukade +14

We report our recent progress on extragalactic spectroscopic and continuum observations, including HCN(J=1-0), HCO(J=1-0), and CN(N=1-0) imaging surveys of local Seyfert and st…

astro-ph2008★ 5 cited

ASTE CO(3--2) Observations of the Southern Barred Spiral Galaxy NGC 986: a Large Gaseous Bar Filled with Dense Molecular Medium

K. Kohno, T. Tosaki, R. Miura +20

We present CO(3-2) emission observations toward the 3'x3' (or 20x20kpc at a distance of 23Mpc) region of the southern barred spiral galaxy NGC 986 using the Atacama Submillimeter T…

astro-ph2007★ 139 cited

On-The-Fly Observing System of the Nobeyama 45-m and ASTE 10-m Telescopes

Tsuyoshi Sawada, Norio Ikeda, Kazuyoshi Sunada +10

We have developed spectral line On-The-Fly (OTF) observing mode for the Nobeyama Radio Observatory 45-m and the Atacama Submillimeter Telescope Experiment 10-m telescopes. Sets of…

astro-ph2007★ 13 cited

The 2006 Radio Outburst of a Microquasar Cyg X-3: Observation and Data

M. Tsuboi, T. Tosaki, N. Kuno +22

We present the results of the multi-frequency observations of radio outburst of the microquasar Cyg X-3 in February and March 2006 with the Nobeyama 45-m telescope, the Nobeyama Mi…

astro-ph2007★ 19 cited

A Complete Survey of the Central Molecular Zone in NH3

Takumi Nagayama, Toshihiro Omodaka, Toshihiro Handa +4

We present a map of the major part of the central molecular zone (CMZ) of simultaneous observations in the NH3 (J,K) = (1,1) and (2,2) lines using the Kagoshima 6-m telescope. The…

astro-ph2005★ 59 cited

The Elongations and Supersonic Motions of Molecular Clouds

Jin Koda, Tsuyoshi Sawada, Tetsuo Hasegawa +1

New 13CO data from the BU-FCRAO Milky Way Galactic Ring Survey (GRS) are analyzed to understand the shape and internal motions of molecular clouds. For a sample of more than five h…