activity
19982015
most citedDust-to-gas ratio, factor and CO-dark gas in the Galactic anticentre: an observational study

39 citations · 86 across the 3 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2015★ 39 cited

Dust-to-gas ratio, factor and CO-dark gas in the Galactic anticentre: an observational study

B. -Q. Chen, X. -W. Liu, H. -B. Yuan +2

We investigate the correlation between extinction and H~{\sc i} and CO emission at intermediate and high Galactic latitudes ($|b|>10\degr$) within the footprint of the Xuyi Schmidt…

astro-ph.GA2014★ 30 cited

RR Lyrae in XSTPS: The halo density profile in the North Galactic Cap

Lorenzo Faccioli, Martin C. Smith, H. -B. Yuan +4

We present a catalog of RR Lyrae stars (RRLs) observed by the Xuyi Schmidt Telescope Photometric Survey (XDSS). The area we consider is located in the North Galactic Cap, covering…

astro-ph.GA2013★ 17 cited

Spectroscopic Observations of Planetary Nebulae in the Northern Spur of M31

X. Fang, Y. Zhang, R. Garcia-Benito +2

We present spectroscopy of three planetary nebulae (PNe) in the Northern Spur of the Andromeda Galaxy (M31) obtained with the Double Spectrograph on the 5.1 m Hale Telescope at the…

astro-ph.HE2012

The extremely long period X-ray source in a young supernova remnant: a Thorne-Zytkow Object descendant?

X. W. Liu, R. X. Xu, E. P. J. van den Heuvel +4

The origin of the 6.67 hr period X-ray source, 1E161348-5055, in the young supernova remnant RCW 103 is puzzling. We propose that it may be the descendant of a Thorne-Zytkow Object…

astro-ph.SR2012

[Fe III] emission lines in the planetary nebula NGC 2392

Y. Zhang, X. Fang, W. Chau +4

NGC 2392 is a young double-shell planetary nebula (PN). Its intrinsic structure and shaping mechanism are still not fully understood. In this paper we present new spectroscopic obs…

astro-ph.SR2011

New effective recombination coefficients for nebular N II lines

X. Fang, P. J. Storey, X. -W. Liu

Here we report new calculations of the effective recombination coefficients for the \ion{N}{ii} recombination spectrum. We have taken into account the density dep…