Chandra studies of the globular cluster 47 Tucanae: a deeper X-ray source catalogue, five new X-ray counterparts to millisecond radio pulsars and new constraints to r-mode instability window
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/472/3/3706/20331257/stx2241.pdf
Reference115 articles.
1. The Frequency of Binary Stars in the Core of 47 Tucanae
2. A new class of radio pulsars
3. Vortex creep and the internal temperature of neutron stars. I - General theory
4. A New Class of Unstable Modes of Rotating Relativistic Stars
5. Strange stars as persistent sources of gravitational waves
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1. Investigating the nature of the 2.4 h-period eclipsing cataclysmic variable W2 in 47 Tuc;Astronomy & Astrophysics;2024-09
2. Simultaneous Chandra and HST observations of the quiescent neutron star low-mass X-ray binaries in 47 Tucanae;Monthly Notices of the Royal Astronomical Society;2024-04-27
3. Instability windows of relativistic r -modes;Physical Review D;2024-02-08
4. Ultradeep ATCA Imaging of 47 Tucanae Reveals a Central Compact Radio Source;The Astrophysical Journal;2024-01-01
5. Low-Mass X-ray Binaries;Handbook of X-ray and Gamma-ray Astrophysics;2024
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