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The magnetic dipole radiation plus wind (MDRW) model for a pulsar successfully explains the evolution of the braking index between 1 and 3, by which we calculate the initial spins of the pulsars with the measured braking index, and obtain their distribution between and ms. This result is ...
Download: Download full-size image Fig. 3. Number of Galactic disk MSPs discovered as a function of time. Primarily due to the surveys with a new generation of highly sensitive telescopes (FAST, MeerKAT), the discovery rate in recent years has remained as high as it has ever been. Data ...
In this review we describe recent observational and theoretical developments in our understanding of pulsar winds and pulsar-wind nebulae (PWNe). We put sp
model_runtime.entities.common_entities import I18nObject 8 + from core.model_runtime.entities.llm_entities import LLMMode, LLMResult, LLMResultChunk, LLMResultChunkDelta 9 + from core.model_runtime.entities.message_entities import ( 10 + AssistantPromptMessage, 11 + ImagePromptMessageContent...