Hadronic gamma-ray images of the simulated T Coronae Borealis outburst

The hadronic gamma-ray images of T Coronae Borealis for a few reference models corresponding to several time moments after explosion in photons with energies 0.1 - 300 GeV. The units are $erg\, s^{-1}\,cm^{-2}$. arXiv preprint: https://arxiv.org/abs/2603.15570 (Fig. 6 and Fig. 8) - accepted by Astronomy & Astrophysics北冕座T星（T Coronae Borealis）的强子伽马射线图像，对应其爆发后数个时刻的若干参考模型，所用光子能量范围为0.1~300 GeV。图像单位为尔格·秒⁻¹·厘米⁻²（erg·s⁻¹·cm⁻²）。arXiv预印本：https://arxiv.org/abs/2603.15570（对应图6与图8），该研究已被《Astronomy & Astrophysics》（《天文学与天体物理学》）录用。