Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights
Investigating the development of pulsars and millisecond pulsars (MSPs) highlights for us statistical insights, important research areas, and unresolved aspects to address. Through the following work, we provide a detailed demographical study of these astrophysical objects by combining data from several observational techniques (radio, X-ray, and gamma-ray) in different environments: Galactic Field (GF) and Globular Clusters (GC).
Authors
- Francesco Flammini Dotti (ORCID: https://orcid.org/0000-0002-8881-3078)
- A. M. Mickaelian (ORCID: https://orcid.org/0000-0002-6598-1060)
- Maria Rah
- Rainer Spurzem (ORCID: https://orcid.org/0000-0003-2264-7203)
Institutions
- Chinese Academy of Sciences (CN)
- Heidelberg University (DE)
- Byurakan Astrophysical Observatory (AM)
- National Astronomical Observatories (CN)
- National Academy of Sciences of Armenia (AM)
Publication Details
- Journal
- Communications of the Byurakan Astrophysical Observatory
- Published
- 2024-12-27
- DOI
- https://doi.org/10.52526/25792776-24.71.2-351
- Citations
- 2
- Primary Topic
- Superconducting Materials and Applications
- Type
- article
- Field-Weighted Citation Impact
- 0.37
Funders
- Deutsche Forschungsgemeinschaft