UPDATES ON THE GLITCHING PULSAR MONITORING CAMPAIGN PERFORMED FROM IAR
Paper in proceeding, 2024
Pulsars are known for their exceptionally stable rotation. However, this stability can be disrupted by glitches, sudden increases in rotation frequency whose cause is poorly understood. In this study, we present some preliminary results from the pulsar monitoring campaign conducted at the IAR since 2019. We present measurements from timing solution fits of the parameters of five glitches: one glitch in the Vela pulsar, one in PSR J0742−2822, one in PSR J1740−3015, and two mini-glitches in PSR J1048−5832. Finally, we applied the vortex creep model to characterize the inter-glitch period of Vela. However, the preliminary results yielded highly degenerate and loosely constrained parameters.
Radio continuum: general
Pulsars: general
Method: data analysis
Author
E. Zubieta
National University of La Plata
Consejo Nacional de Investigaciones Cientificas y Tecnicas
Santiago Del Palacio
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
Consejo Nacional de Investigaciones Cientificas y Tecnicas
Federico García
Consejo Nacional de Investigaciones Cientificas y Tecnicas
S. B. Araujo Furlan
Astronomía
Instituto de Astronomía Teórica y Experimental (IATE)
G. Gancio
Consejo Nacional de Investigaciones Cientificas y Tecnicas
Carlos O. Lousto
Rochester Institute of Technology
J. A. Combi
Universidad de Jaén
Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
14052059 (ISSN)
Vol. 56 161-165
2022 Instituto Argentino de Radioastronomia (IAR) 60th Anniversary: Prospects for Low-Frequency Radio Astronomy in South America
Buenos Aires, Argentina,
Buenos Aires, Argentina,
Subject Categories
Astronomy, Astrophysics and Cosmology
DOI
10.22201/ia.14052059p.2024.56.29