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EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8–6.3

  • Authors: Miroslav D. Filipović, Shi Dai, Bojan Arbutina, Natasha Hurley-Walker, Robert Brose, Werner Becker, Hidetoshi Sano, Dejan Urošević, T. H. Jarrett, Andrew M. Hopkins, Rami Z. E. Alsaberi, R. Alsulami, Cristobal Bordiu, Brianna Ball, Filomena Bufano, Christopher Burger-Scheidlin, Evan Crawford, Jayanne English, Frank Haberl, Adriano Ingallinera, Anna D. Kapinska, Patrick J. Kavanagh, Bärbel S. Koribalski, Roland Kothes, Sanja Lazarević, Jonathan Mackey, Gavin Rowell, Denis Leahy, Sara Loru, Peter J. Macgregor, Luciano Nicastro, Ray P. Norris, Simone Riggi, Manami Sasaki, Milorad Stupar, Corrado Trigilio, Grazia Umana, Tessa Vernstrom, Branislav Vukotić

Miroslav D. Filipović et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 7.

RGB image of G288.8–6.3 as seen in the eROSITA all-sky surveys eRASS:5. Photons to produce the image were color-coded according to their energy (red for energies 0.2–0.7 keV, green for 0.7–1.2 keV, blue for 1.2–2.4 keV). An adaptive kernel smoothing algorithm was applied to the images in each energy band. Radio contour lines (green: 0.1, 0.2, 0.5, and 1 mJy beam−1) are overlaid to mark the outline of G288.8–6.3. The positions of the neighboring radio pulsar PSR J1036–6559 and the Fermi source 4FG J1028.7–6431c are shown.

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