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Constraints on the X-ray and Very High Energy $γ$-ray Flux from Supernova Remnant W44

Fuente: arXiv

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Bibliographic Details
Main Authors:	Archer, A., Bangale, P., Bartkoske, J. T., Benbow, W., Buckley, J. H., Chen, Y., Christiansen, J. L., Chromey, A. J., Duerr, A., Errando, M., Godoy, M. Escobar, Feldman, S., Feng, Q., Foote, J., Fortson, L., Furniss, A., Hanlon, W., Hervet, O., Hinrichs, C. E., Holder, J., Humensky, T. B., Jin, W., Johnson, M. N., Kaaret, P., Kertzman, M., Kherlakian, M., Kieda, D., Kleiner, T. K., Korzoun, N., Kumar, S., Kundu, S., Lang, M. J., Maier, G., Lundy, M., Millard, M. J., Mooney, C. L., Moriarty, P., Mukherjee, R., Ning, W., Ong, R. A., Pohl, M., Pueschel, E., Quinn, J., Rabinowitz, P. L., Ragan, K., Reynolds, P. T., Ribeiro, D., Roache, E., Saha, L., Santander, M., Sembroski, G. H., Shang, R., Tak, D., Talluri, A. K., Tucci, J. V., Williams, D. A., Wong, S. L., Woo, J.
Format:	Preprint
Published:	2025
Subjects:	High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2503.09778