Nature of the Diffuse Source and Its Central Point-like Source in SNR 0509-67.5

Nature of the Diffuse Source and Its Central Point-like Source in SNR 0509-67.5

We examine a diffuse emission region near the center of SNR 0509-67.5 to determine its nature. Within this diffuse region we observe a point-like source that is bright in the near-IR, but is not visible in the B and V bands. We consider an emission line observed at 6766 angstrom and the possibilitie...

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Bibliographic Details
Main Authors: Litke, Katrina C., Chu, You-Hua, Holmes, Abigail, Santucci, Robert, Blindauer, Terrence, Gruendl, Robert A., Li, Chuan-Jui, Pan, Kuo-Chuan, Ricker, Paul M., Weisz, Daniel R.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
ISM: individual objects (SNR 0509-67.5)
ISM: supernova remnants
Magellanic Clouds
Online Access:http://hdl.handle.net/10150/624374
http://arizona.openrepository.com/arizona/handle/10150/624374

Internet

http://hdl.handle.net/10150/624374
http://arizona.openrepository.com/arizona/handle/10150/624374

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