Peer-reviewedPublisher termsAstronomy & Astrophysics
Chemical complexity in feedback from supernova remnants: First detection of PO+ in IC443 and W44
Related
- Measuring Small-scale Turbulence in Supernova Remnants with Jitter Radiation
- Estimation of Dust Mass from Infrared Emission and Extinction of Supernova Remnants: G93.7-0.2, G109.1-1.0, G156.2+5.7, and G166.0+4.3
- Estimation of Dust Mass from Infrared Emission and Extinction of Supernova Remnants: G93.7−0.2, G109.1−1.0, G156.2+5.7, and G166.0+4.3
- The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants
- Optical Discovery of New and Candidate Galactic Supernova Remnants Plus Optical Imaging of the Monogem Supernova Remnant
BibTeX
@article{cosentino2026chemical,
title = {{Chemical complexity in feedback from supernova remnants: First detection of PO+ in IC443 and W44}},
author = {G. Cosentino and F. D. Priestley and S. Scibelli and F. Fontani},
journal = {Astronomy \& Astrophysics},
year = {2026},
month = oct,
doi = {10.1051/0004-6361/202661028},
url = {https://www.aanda.org/10.1051/0004-6361/202661028},
}
RIS
TY - JOUR
TI - Chemical complexity in feedback from supernova remnants: First detection of PO+ in IC443 and W44
AU - G. Cosentino
AU - F. D. Priestley
AU - S. Scibelli
AU - F. Fontani
PY - 2026
DA - 2026/10/06
JO - Astronomy & Astrophysics
DO - 10.1051/0004-6361/202661028
UR - https://www.aanda.org/10.1051/0004-6361/202661028
SN - 0004-6361
SN - 1432-0746
ER -