activity
20122026
most citedConsiderations for a Multi-beam Multi-purpose Survey with FAST

314 citations · 1.3k across the 55 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2025

Tomography of the Ophiuchus Molecular Cloud with Velocity Features in CH spectra: A Pilot Study of Coherent Sub-structures

Lei qian, Zhichen Pan, Dongyue Jiang +1

The CH transition was used to investigate the possible line of sight sub-structures from the dense and optically thick in CO regions in the Ophiuchus sta…

astro-ph.GA2018★ 58 cited

Where is OH and Does It Trace the Dark Molecular Gas (DMG)?

Di Li, Ningyu Tang, Hiep Nguyen +15

Hydroxyl (OH) is expected to be abundant in diffuse interstellar molecular gas as it forms along with under similar conditions and within a similar extinction range. We have…

astro-ph.GA2017★ 3 cited

Water abundance in four of the brightest water sources in the southern sky

Bing-Ru Wang, Lei Qian, Di Li +1

We estimated the ortho-{\rm{HO}} abundances of G267.9--1.1, G268.4--0.9, G333.1--0.4 and G336.5--1.5, four of the brightest ortho-{\rm{HO}} sources in the southern sky obse…

astro-ph.GA2017★ 14 cited

Large-Scale Spectroscopic Mapping of the Ophiuchi Molecular Cloud Complex I. The CH to NH Ratio as a Signpost of Cloud Characteristics

Zhichen Pan, Di Li, Qiang Chang +3

We present 2.5-square-degree CH N=1-0 and NH J=1-0 maps of the Ophiuchi molecular cloud complex. These are the first large-scale maps of the Ophiuchi molecula…

astro-ph.GA2016★ 29 cited

Physical properties of CO-dark molecular gas traced by C

Ningyu Tang, Di Li, Carl Heiles +3

Neither HI nor CO emission can reveal a significant quantity of so-called dark gas in the interstellar medium (ISM). It is considered that CO-dark molecular gas (DMG), the molecula…

astro-ph.GA2015★ 22 cited

A New Method for Constraining Molecular Cloud Thickness: A study of Taurus, Perseus and Ophiuchus

Lei Qian, Di Li, Stella Offner +1

The core velocity dispersion (CVD) is a potentially useful tool for studying the turbulent velocity field of molecular clouds. CVD is based on centroid velocities of dense gas clum…

astro-ph.GA2015

Quantifying Dark Gas

Di Li, Duo Xu, Carl Heiles +2

A growing body of evidence has been supporting the existence of so-called "dark molecular gas" (DMG), which is invisible in the most common tracer of molecular gas, i.e., CO rotati…