activity
20162026
most citedThe FAST all sky HI survey (FASHI): The first release of catalog

83 citations · 345 across the 37 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 2 cited

The environment and star formation of HII region Sh2-163: a multi-wavelength study

Naiping Yu, Jun-Jie Wang, Nan Li

To investigate the environment of HII region Sh2-163 and search for evidence of triggered star formation in this region, we performed a multi-wavelength study of this HII region. M…

astro-ph.GA2016★ 6 cited

Physical and chemical properties of Red MSX Sources in the southern sky: HII regions

Naiping Yu, Jun-Jie Wang, Nan Li

We have studied the physical and chemical properties of 18 southern Red Midcourse Space Experiment Sources (RMSs), using archival data taken from the Atacama Pathfinder Experiment…

astro-ph.GA2016★ 1 cited

A multiwavelength study of the star forming H II region Sh2-82

Nai-Ping Yu Jun-Jie Wang

Based on a multiwavelength study, the interstellar medium and young stellar objects (YSOs) around the HII region Sh2-82 have been analyzed. Two molecular clumps were found from the…

astro-ph.GA2016★ 5 cited

A multi-transition molecular line study of infrared dark cloud G331.71+00.59

Nai-Ping Yu, Jun-Jie Wang

Using archive data from the Millimeter Astronomy Legacy Team Survey at 90 GHz (MALT90), carried out using the Mopra 22-m telescope, we made the first multi-transition molecular lin…

astro-ph.GA2016★ 24 cited

A molecular line study towards massive extended green object clumps in the southern sky: chemical properties

Naiping Yu, Jun-Jie Wang

We present a molecular line study towards 31 extended green object (EGO) clumps in the southern sky using data from MALT90 (Millimetre Astronomy Legacy Team 90 GHz). According to p…

astro-ph.GA2016★ 8 cited

Molecular line study of massive star forming regions from the RMS survey

Naiping Yu, Jun Jie Wang

In this paper we selected a sample of massive star forming regions from the Red MSX Source (RMS) survey, to study star formation activities (mainly outflow and inflow signatures).