activity
20002023
most citedThe Dynamic Evolution of Young Extragalactic Radio Sources

215 citations · 1.6k across the 63 of their papers we have counts for

collaborators

65 papers

astro-ph.GA2023

VLBI Observations of a sample of Palomar-Green quasars II: characterising the parsec-scale radio emission

Ailing Wang, Tao An, Yingkang Zhang +4

This study uses multi-frequency Very Long Baseline Interferometry (VLBI) to study the radio emission from 10 radio-quiet quasars (RQQs) and four radio-loud quasars (RLQs). The dive…

astro-ph.GA2023★ 16 cited

Gravitational collapse and accretion flows in the hub filament system G323.46-0.08

Yingxiu Ma, Jianjun Zhou, Jarken Esimbek +9

We studied the hub filament system G323.46-0.08 based on archival molecular line data from the SEDIGISM 13CO survey and infrared data from the GLIMPSE, MIPS, and Hi-GAL surveys. G3…

astro-ph.GA2023★ 4 cited

The OH Megamaser Emission in Arp\,220: the rest of the story

W. A. Baan, J. N. H. S. Aditya, T. An +1

The OH Megamaser emission in the merging galaxy Arp220 has been re-observed with the Multi-Element Radio Linked Interferometer Network (MERLIN) and the European VLBI Network (EVN).…

astro-ph.GA2023

Off-nuclear H2O maser and dense molecular gas in NGC1068

Yoshiaki Hagiwara, Willem A. Baan, Masatoshi Imanishi +1

The results of high-resolution spectral-line observations of dense molecular gas are presented towards the nuclear region of the type 2 Seyfert galaxy NGC1068. MERLIN observations…

astro-ph.HE2023★ 1 cited

Unveiling the small-scale jets in the rapidly growing supermassive black hole IZw1

Xiaolong Yang, Su Yao, Luigi C. Gallo +10

Accretion of black holes at near-Eddington or super-Eddington rates is the most powerful episode that drives black hole growth, and it may work in several types of objects. However…

astro-ph.GA2023★ 10 cited

Mildly Relativistic Motion in the Radio Quiet Quasar PG 1351+640

Ailing Wang, Tao An, Shaoguang Guo +8

Measuring the proper motion of the emission component in radio-quiet quasars (RQQs) could help to distinguish between the origins of the radio emission and to understand whether th…