activity
20002026
most citedSMA CO(J=3-2) interferometric observations of the central region of M51

60 citations · 183 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

First Submillimeter Lights from Dome A: Tracing the Carbon Cycle in the Feedback of Massive Stars

Yan Gong, Jiaqiang Zhong, Yuan Ren +38

The cycling of carbon between its ionized, atomic, and molecular phases shapes the chemical compositions and physical conditions of the interstellar medium (ISM). However, ground-b…

astro-ph.GA2025★ 1 cited

The Milky Way Imaging Scroll Painting Survey: Data Release 1

Ji Yang, Qing-Zeng Yan, Yang Su +31

We present the first data release (DR1) of the Milky Way Imaging Scroll Painting (MWISP) survey, a mapping in the J=(1-0) transition lines of 12CO, 13CO, and C18O toward the northe…

astro-ph.SR2017★ 41 cited

L1188: a promising candidate of cloud-cloud collision triggering the formation of the low- and intermediate-mass stars

Yan Gong, Min Fang, Ruiqing Mao +7

We present a new large-scale (4 square degrees) simultaneous CO, CO, and CO (=10) mapping of L1188 with the PMO 13.7-m telescope. Our observations have r…

astro-ph.GA2016★ 26 cited

Molecular clouds and star formation toward the Galactic plane within 216.25 l 218.75 and 0.75 b 1.25

Y. Gong, R. Q. Mao, M. Fang +9

As a part of the Milky Way Imaging Scroll Painting (MWISP) survey, we performed a simultaneous 12CO(1-0), 13CO(1-0), C18O(1-0) mapping toward molecular clouds in a region encompass…

astro-ph2006★ 45 cited

Detection of CO Hotspots Associated with Young Clusters in the Southern Starburst Galaxy NGC 1365

Kazushi Sakamoto, Paul T. P. Ho, Rui-Qing Mao +2

We have used the Submillimeter Array for the first interferometric CO imaging toward the starburst-Seyfert nucleus of the southern barred spiral galaxy NGC 1365, which is one of th…

astro-ph2004★ 60 cited

SMA CO(J=3-2) interferometric observations of the central region of M51

S. Matsushita, K. Sakamoto, C. -Y. Kuo +9

We present the first interferometric CO(J=3-2) observations (beam size of 3.9"x1.6" or 160pc x 65pc) with the Submillimeter Array (SMA) toward the center of the Seyfert 2 galaxy M5…