Peer-reviewedPublisher termsAstronomy & Astrophysics
On the mean profiles of radio pulsars. III. Identifying the mode
Related
- Nonbirefringent model of orthogonal polarization modes in radio pulsars - New view on S swing and mode structure in pulsar beam
- Interior Magnetic Fields in Magnetars and Radio Pulsars
- Observational selection effects on radio pulsars are minimal for masses, but significant for orbits and spins
- Connecting radio pulsars, magnetars, and XDINSs in a unified evolutionary framework using simulation-based inference
- Pulse profiles of tall accretion columns in X-ray pulsars
BibTeX
@article{jaroenjittichai2026mean,
title = {{On the mean profiles of radio pulsars. III. Identifying the mode}},
author = {P. Jaroenjittichai and A. A. Philippov and V. S. Beskin and M. Kramer and A. Yu. Istomin and F. A. Kniazev},
journal = {Astronomy \& Astrophysics},
year = {2026},
month = oct,
doi = {10.1051/0004-6361/202660622},
url = {https://www.aanda.org/10.1051/0004-6361/202660622},
}
RIS
TY - JOUR
TI - On the mean profiles of radio pulsars. III. Identifying the mode
AU - P. Jaroenjittichai
AU - A. A. Philippov
AU - V. S. Beskin
AU - M. Kramer
AU - A. Yu. Istomin
AU - F. A. Kniazev
PY - 2026
DA - 2026/10/31
JO - Astronomy & Astrophysics
DO - 10.1051/0004-6361/202660622
UR - https://www.aanda.org/10.1051/0004-6361/202660622
SN - 0004-6361
SN - 1432-0746
ER -