3 papers
astro-ph.GA2019
The kinematic distances of SNR G16.7+0.1 and G15.9+0.2 by analyzing HI absorption spectra
W. W. Tian, H. Zhu, M. F. Zhang +3
We build HI absorption spectra towards Supernova Remnant (SNRs) G16.7+0.1 and G15.9+0.2 using the THOR survey data. With the absorption spectra, we give a new distance range of 7 t…
astro-ph.GA2019
Dust destruction in non-radiative shocks
H. Zhu, P. Slane, J. Raymond +1
Supernova remnant (SNR) shock waves are the main place where interstellar dust grains are destroyed. However, the dust destruction efficiency in non-radiative shocks is still not w…
astro-ph.HE2015
Suzaku observation and distance of supernova remnant G332.5-5.6
H. Zhu, W. W. Tian, D. Wu
We analyze the Suzaku XIS data of the central region of supernova remnant G332.5-5.6. The X-ray data are well described by a single non-equilibrium ionization thermal model, {\tt v…