Peer-reviewedPublisher termsAstronomy & Astrophysics
Possible origins of the two γ-ray components C0 and C1 in IC 443
Related
- Diversity of planetary origins and compositions traced by stellar abundance differences among co-natal star systems
- 4U 1624-490 as a possible intermediate-mass X-ray binary: Constraints from XRISM and NuSTAR spectroscopy
- Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider
- Second-scale periodicity in FRB 20201124A: Coincident with critical rotation measure evolution epochs and its possible implication
- The multiple origins of spurs in stellar streams: a challenge for dark matter diagnostics
BibTeX
@article{xian2026possible,
title = {{Possible origins of the two γ-ray components C0 and C1 in IC 443}},
author = {Yujun Xian and Huan Yu and Bo Wang and Jun Fang},
journal = {Astronomy \& Astrophysics},
year = {2026},
month = nov,
doi = {10.1051/0004-6361/202662084},
url = {https://www.aanda.org/10.1051/0004-6361/202662084},
}
RIS
TY - JOUR
TI - Possible origins of the two γ-ray components C0 and C1 in IC 443
AU - Yujun Xian
AU - Huan Yu
AU - Bo Wang
AU - Jun Fang
PY - 2026
DA - 2026/11/03
JO - Astronomy & Astrophysics
DO - 10.1051/0004-6361/202662084
UR - https://www.aanda.org/10.1051/0004-6361/202662084
SN - 0004-6361
SN - 1432-0746
ER -