The origin of recombining plasma and the detection of the Fe-K line in the supernova remnant W 28.

MLA

Hiromichi OKON, et al. “The Origin of Recombining Plasma and the Detection of the Fe-K Line in the Supernova Remnant W 28.” Publications of the Astronomical Society of Japan, vol. 70, no. 3, June 2018, p. 35–1–N.PAG. EBSCOhost, https://doi.org/10.1093/pasj/psy022.

APA

Hiromichi OKON, Hiroyuki UCHIDA, Takaaki TANAKA, Hideaki MATSUMURA, & Takeshi Go TSURU. (2018). The origin of recombining plasma and the detection of the Fe-K line in the supernova remnant W 28. Publications of the Astronomical Society of Japan, 70(3), 35–1–N.PAG. https://doi.org/10.1093/pasj/psy022

Chicago

Hiromichi OKON, Hiroyuki UCHIDA, Takaaki TANAKA, Hideaki MATSUMURA, and Takeshi Go TSURU. 2018. “The Origin of Recombining Plasma and the Detection of the Fe-K Line in the Supernova Remnant W 28.” Publications of the Astronomical Society of Japan 70 (3): 35–1–N.PAG. doi:10.1093/pasj/psy022.