An Investigation of the Interstellar Environment of Supernova Remnant CTB 87

22 May 2018 Liu Qian-Cheng Chen Yang Chen Bing-Qiu Zhou Ping Wang Xiao-Tao Su Yang

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 coincident surrounding superbubble. The CO observation shows that the SNR delineated by the radio emission is projectively covered by a molecular cloud (MC) complex at V$_{\rm {LSR}}$ = $-60$ to $-54$ km s$^{-1}$... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • ASTROPHYSICS OF GALAXIES