139 citations · 1.9k across the 77 of their papers we have counts for
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FERMI observation of the jets of the microquasar SS433
Yi Xing, Zhongxiang Wang, Xiao Zhang +2
We report our analysis of the data obtained with the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope (Fermi) for the SS 433/W50 region. The total data length…
Searching for GeV gamma-ray emission from the bulge of M31
Li Feng, Zhiyuan Li, Meng Su +2
The three major large-scale, diffuse -ray structures of the Milky Way are the Galactic disk, a bulge-like GeV excess towards the Galactic center, and the Fermi bubble. Whether s…
Molecular gas toward supernova remnant Cassiopeia A
Ping Zhou, Jiang-Tao Li, Zhi-Yu Zhang +5
We mapped 12CO J=1-0, 12CO J=2-1, 13CO J=1-0, and 13CO J=2-1 lines toward supernova remnant (SNR) Cassiopeia A with the IRAM 30m telescope. The molecular clouds (MCs) along the lin…
Spatially resolved broad-band synchrotron emission from the non-thermal limbs of SN1006
Jiang-Tao Li, Jean Ballet, Marco Miceli +6
We present ~400ks NuSTAR observations of the northeast (NE) and southwest (SW) non-thermal limbs of the Galactic SNR SN1006. We discovered three sources with X-ray emission detecte…
The Large-scale ISM of SS433/W50 Revisited
Yang Su, Xin Zhou, Ji Yang +3
With new high-resolution CO and HI data, we revisited the large-scale interstellar medium (ISM) environment toward the SS 433/W50 system. We find that two interesting molecular clo…
Resonant scattering effect on the soft X-ray line emission from the hot interstellar medium: I. galactic bulges
Yang Chen, Q. Daniel Wang, Gao-Yuan Zhang +2
Diffuse soft X-ray line emission is commonly used to trace the thermal and chemical properties of the hot interstellar medium, as well as its content, in nearby galaxies. Although…
An Investigation of the Interstellar Environment of Supernova Remnant CTB 87
Qian-Cheng Liu, Yang Chen, Bing-Qiu Chen +3
We present a new millimeter CO-line observation towards supernova remnant (SNR) CTB 87, which was regarded purely as a pulsar wind nebula (PWN), and an optical investigation of a c…