Conveners
Parallel 1: Pulsar I
- Christo Venter
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Dr Pablo Saz Parkinson (University of California, Santa Cruz)10/10/2022, 16:00Contributed Talk
The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is a Chinese megascience facility built by the National Astronomical Observatories (NAOC) of the Chinese Academy of Sciences (CAS). Completed in 2016, FAST is the world's largest single-dish radio telescope, and is currently operating as an international facility, with regular proposal calls open to observers from around the...
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10/10/2022, 16:15
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Addy Evans10/10/2022, 16:30Contributed Talk
There are now 35 confirmed gamma-ray bright globular clusters (GCs) in the Milky Way. The millisecond pulsar (MSP) populations within these clusters are widely considered to be their primary source of gamma-ray emission. There are two proposed mechanisms for high-energy gamma-rays to be created in GCs by MSPs. The first is radiation from charged particles traveling along the open magnetic...
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Andrey Timokhin (University of Zielona Góra)10/10/2022, 16:45Contributed Talk
For more than five decades, the origin of pulsar radio emission have been one of the
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major unsolved problems in astrophysics. It is universally believed that generation
of radio emission is intimately connected with pair plasma production initiated by
high energy gamma-rays in pulsar polar caps. Here I will present the results of our
study of electron-positron pairs creation near magnetic... -
10/10/2022, 17:00
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Anu Kundu10/10/2022, 17:15Contributed Talk
The Neutron star Interior Composition Explorer (NICER) has been operating since 2017 with the major aim of gaining a better understanding of the extreme nature of neutron stars (NSs). With its exceptional sensitivity, it hopes to constrain the equation of state of NSs to high precision. Modelling thermal X-ray light curves (LCs) of pulsars can provide us with insights into the magnetic field...
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Massimiliano RazzanoContributed Talk
PSR J2021+4026 in the Cygnus region is one of the most interesting radio-quiet pulsars detected by Fermi-LAT. This source, thought to be associated with the Gamma Cygni supernova remnant, is the first isolated gamma-ray pulsar that exhibited clear evidence of variability, with a simultaneous flux and spindown change first occurred in October 2011. After a long recovery phase, in August 2015...
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Dr Zorawar Wadiasingh (University of Maryland College Park/ NASA GSFC / NWU)Contributed Talk
Fermi GBM has a catalog of many hundreds of magnetar bursts. These bursts are short in duration, quasi-thermal in spectrum and exhibit complex spectro-temporal behavior suggestive of Comptonized fireballs. Recent report of rotational-phase selection of magnetar short bursts in SGR 1830-0645 and SGR 1935+2154 strongly suggest a fixed and low altitude emission locale for magnetic flux tubes...
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