HEASA 2021

Session

Pulsars I

16 Sept 2021, 16:00

Conveners

Pulsars I

• Nukri Komin (University of the Witwatersrand, Johannesburg, South Africa)

130. Modeling globular clusters as multi-wavelength emitters

Hambeleleni Davids (University of Namibia, North-West University)

16/09/2021, 16:00

Pulsars

Dissertation talk

At present, only a single Globular Cluster (GC) has plausibly been detected at very high energies (VHEs) by H.E.S.S. The future CTA is expected to detect more GCs in this band. We present results from an emission code that assumes millisecond pulsars (MSPs) to be sources of relativistic particles diffusing through GCs that will give broad-band radiation due to their interaction with the...

131. Constraining the magnetic field geometry of the millisecond pulsar PSR J0030+0451 using NICER and Fermi data

Anu Kundu (NWU)

16/09/2021, 16:25

Pulsars

Contributed talk

The Neutron star Interior Composition Explorer (NICER) was installed aboard the International Space Station (ISS) in 2017 with the major aim of gaining a better understanding of the extreme nature and composition of neutron stars (NSs). With its exceptional sensitivity, it hopes to constrain the equation of state for these compact objects to high precision. Modelling thermal X-ray light curves...

132. Constraining the non-thermal emission site and geometry of AR Sco via optical po- larimetry

Louis Du Plessis (Centre for Space Physics, North-West University)

16/09/2021, 16:40

Pulsars

Contributed talk

Marsh et al. detected radio and optical pulsations from the binary system AR Scorpii (AR Sco). This system, with an orbital period of 3.55 h, is composed of a cool, low-mass star and a white dwarf (WD) with a spin period of 1.95 min. Takata et al. also detected X-ray pulsations from this source. These observations indicate no presence of an accretion disk or column. Buckley et al. found that...

133. Low power pulsed emission at the spin period of the WD in AR Scorpii?

Quinton Kaplan (University of the Free State)

16/09/2021, 16:55

Pulsars

Contributed talk

Previous studies indicate that AR Sco’s surrounding region complicates the search for Gamma-ray emission from this source. The fact that AR Sco lies close to the Galactic plane and strong nearby VHE Fermi sources, make it difficult to constrain and quantify an upper-limit of the emission from AR Sco’s location in the sky. In this study, a search for high energy gamma-ray emission was...

134. The detection of pulsed emission at the spin period of the white dwarf in AE Aquarii in MeerKAT and Fermi-LAT data

Spencer Tendai Madzime (University of the Free State)

16/09/2021, 17:10

Pulsars

Contributed talk

Here we present the first report of pulsed emission at the spin period of the white dwarf in MeerKAT data, which is also the first report of pulsed emission at the spin period of the white dwarf in radio frequencies (L-band). Further support for the pulsar-like behaviour of AE Aqr is the detection of pulsed emission at the spin period of the white dwarf in AE Aqr in Fermi-LAT data. By...

135. Pulsar high-energy emission models

Alice Harding (Los Alamos National Laboratory)

16/09/2021, 17:25

Pulsars

Invited talk

Ground-based Air-Cherenkov telescopes have detected pulsations at energies above 50 GeV from a growing number of Fermi pulsars. These include the Crab, Vela, PSR B1706-44 and Geminga, with the first two having pulsed detections above 1 TeV. There appears to be VHE emission that is an extension of the Fermi spectra to high energies as well as additional higher-energy components that require a...