activity
20172022
most citedThe Distances to Molecular Clouds at High Galactic Latitudes based on GAIA DR2

58 citations · 107 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.IM20224 cited

Sciences with Thai National Radio Telescope

Phrudth Jaroenjittichai, Koichiro Sugiyama, Busaba H. Kramer +44

This White Paper summarises potential key science topics to be achieved with Thai National Radio Telescope (TNRT). The commissioning phase has started in mid 2022. The key science…

astro-ph.GA201926 cited

Parallaxes for star forming regions in the inner Perseus spiral arm

Bo Zhang, Mark J. Reid, Lian Zhang +8

We report trigonometric parallax and proper motion measurements of 6.7-GHz CH3OH and 22-GHz H2O masers in eight high-mass star-forming regions (HMSFRs) based on VLBA observations a…

astro-ph.GA201958 cited

The Distances to Molecular Clouds at High Galactic Latitudes based on GAIA DR2

Qing-Zeng Yan, Bo Zhang, Ye Xu +4

We report the distances of molecular clouds at high Galactic latitudes (|b|>10) derived from parallax and G band extinction (A) measurements in the second Gaia da…

astro-ph.GA2018

Improved Selection Criteria for HII Regions, based on IRAS Sources

Qing-Zeng Yan, Ye Xu, A. J. Walsh +6

We present new criteria for selecting HII regions from the Infrared Astronomical Satellite (IRAS) Point Source catalogue (PSC), based on an HII region catalogue derived manually fr…

astro-ph.GA20175 cited

SiO Maser Survey towards off-plane O-rich AGBs around the orbital plane of the Sagittarius Stellar Stream

Yuanwei Wu, Noriyuki Matsunaga, Ross A. Burns +1

We conducted an SiO maser survey towards 221 O-rich AGB stars with the aim of identifying maser emission associated with the Sagittarius stellar stream. In this survey, maser emiss…

astro-ph.GA201714 cited

Towards a three-dimensional distribution of the molecular clouds in the Galactic Centre

Qing-Zeng Yan, A. J. Walsh, J. R. Dawson +8

We present a study of the three-dimensional structure of the molecular clouds in the Galactic Centre (GC) using CO emission and OH absorption lines. Two CO isotopologue lines, $^{1…