activity
20032022
most citedChemical abundances for Hf 2-2, a planetary nebula with the strongest known heavy element recombination lines

98 citations · 354 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2022★ 42 cited

Peering into the Young Planetary System AB Pic. Atmosphere, Orbit, Obliquity & Second Planetary Candidate

P. Palma-Bifani, G. Chauvin, M. Bonnefoy +24

We aim to revisit the system AB Pic which has a known companion at the exoplanet/ brown-dwarf boundary. We based this study on a rich set of observations to investigate the compani…

astro-ph.GA2022★ 22 cited

Radio-loud Quasars above Redshift 4: VLBI Imaging of an Extended Sample

M. Krezinger, K. Perger, K. É. Gabányi +7

High-redshift radio sources provide plentiful opportunities for studying the formation and evolution of early galaxies and supermassive black holes. However, the number of known ra…

astro-ph.SR2015★ 27 cited

DA white dwarfs from the LSS-GAC survey DR1: the preliminary luminosity and mass functions and formation rate

A. Rebassa-Mansergas, X. -W. Liu, R. Cojocaru +9

Modern large-scale surveys have allowed the identification of large numbers of white dwarfs. However, these surveys are subject to complicated target selection algorithms, which ma…

astro-ph2007★ 9 cited

Temperature fluctuations in H II regions: t2 for the two-phase model

Y. Zhang, B. Ercolano, X. -W. Liu

Aims: We investigate temperature fluctuations in H II regions in terms of a two-phase model, which assumes that the nebular gas consists of a hot and a cold phase. Methods: We deri…

astro-ph2006★ 4 cited

Fe/Ni ratio in the Ant Nebula Mz 3

Y. Zhang, X. -W. Liu

We have analyzed the [Fe II] and [Ni II] emission lines in the bipolar planetary nebula Mz~3. We find that the [Fe II] and [Ni II] lines arise exclusively from the central regions.…

astro-ph2006★ 98 cited

Chemical abundances for Hf 2-2, a planetary nebula with the strongest known heavy element recombination lines

X. -W. Liu, M. J. Barlow, Y. Zhang +2

We present high quality optical spectroscopic observations of the planetary nebula (PN) Hf 2-2. The spectrum exhibits many prominent optical recombination lines (ORLs) from heavy e…