activity
20052023
most citedThe Bar and Spiral Arms in the Milky Way: Structure and Kinematics

57 citations · 148 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202313 cited

The parallax and 3D kinematics of water masers in the massive star-forming region G034.43+0.24

Xiaofeng Mai, Bo Zhang, M. J. Reid +12

We report a trigonometric parallax measurement of 22 GHz water masers in the massive star-forming region G034.43+0.24 as part of the Bar and Spiral Structure Legacy (BeSSeL) Survey…

astro-ph.GA20228 cited

A Milliarcsecond-accurate Position for Sagittarius A*

Shuangjing Xu, Bo Zhang, Mark J. Reid +3

The absolute position of Sgr A*, the compact radio source at the center of the Milky Way, had been uncertain by several tens of milliarcseconds. Here we report improved astrometric…

astro-ph.GA202057 cited

The Bar and Spiral Arms in the Milky Way: Structure and Kinematics

Juntai Shen, Xing-Wu Zheng

The Milky Way is a spiral galaxy with the Schechter characteristic luminosity , thus an important anchor point of the Hubble sequence of all spiral galaxies. Yet the true appe…

astro-ph.GA20206 cited

The radio properties of the OH megamaser galaxy IRAS 02524+2046

Hao Peng, Zhongzu Wu, Bo Zhang +7

We present results from VLBI observations of continuum and OH line emission in IRAS 02524+2046 and also arcsecond-scale radio properties of this galaxy using VLA archive data. We f…

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.GA2018

Extended ammonia observations towards the 'Integral-Shaped Filament'

Gang Wu, Keping Qiu, Jarken Esimbek +4

Recent observations suggest a scenario in which filamentary structures in the ISM represent the first step towards clumps/cores and eventually star formation. The densest filaments…