NuSTAR Analysis of the 2024 Periastron Passage of TeV Binary PSR B1259-63
PSR B1259-63 is a well-studied TeV binary, with an energetic pulsar in orbit around a Be star. Using Nuclear Spectroscopic Telescope Array observations during the 2024 passage of the pulsar through the circumstellar disk, we find the spectrum to be the most energetic (Γ = 1.5) around 27 days after p...
Saved in:
Main Authors: | Oliver J. Roberts, Philip Kaaret, M. Lynne Saade, Chien-Ting Chen, Steven R. Ehlert, Ioannis Liodakis, Martin C. Weisskopf |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/adec6a |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
NuSTAR and XMM-Newton Observations of PSR J1930+1852 and Its Pulsar Wind Nebula
by: J. A. J. Alford, et al.
Published: (2025-01-01) -
Investigating the Anticorrelation between Photon Index and Flux of the Crab Using RXTE and NuSTAR
by: Debjit Chatterjee, et al.
Published: (2025-01-01) -
Long-term Astrometric Monitoring of the Galactic Center Magnetar PSR J1745−2900
by: Geoffrey C. Bower, et al.
Published: (2025-01-01) -
Timing Results of 22 yr for PSR J0922+0638
by: Peng Liu, et al.
Published: (2025-01-01) -
Multifrequency Behaviour of the Gamma-Ray Binary System PSR B1259-63: Modelling the FERMI Flare
by: Brian van Soelen, et al.
Published: (2014-12-01)