Discovery of 11 Hz burst oscillations from the 11 Hz Eclipsing Pulsar in Terzan 5

Bibcode
2010ATel.2932....1A
Altamirano, D.; Watts, A.; Kalamkar, M.; Homan, J.; Yang, Y.; Casella, P.; Linares, M.; Patruno, A.; Armas-Padilla, M.; Cavecchi, Y.; Degenaar, N.; Kaur, R.; van der Klis, M.; Rea, N.; Wijnands, R.
Bibliographical reference

The Astronomer's Telegram, #2932

Advertised on:
10
2010
Number of authors
15
IAC number of authors
0
Citations
18
Refereed citations
16
Description
An RXTE pointed observation of the ongoing outburst of of the transient source in the globular cluster Terzan 5 (ATEL #2919, #2920, #2922, #2924, #2929) began at approximately 2010-10-13 at 00:13 UTC, for an exposure of 3.2 ksec. This observation revealed strong pulsations at a barycentric frequency of 11.0452(2) Hz as well as one Type I X-ray burst (Atel #2929). In a detailed analysis of the X-ray burst we find strong burst oscillations at the non-barycentered frequency of ~11.05 Hz, consistent with the spin frequency of this neutron star.
Type
Non-refereed

It may interest you

  • Non-refereed
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Advertised on:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Citations
    0
  • Non-refereed
    Co-phasing the distributed aperture of a Fizeau interferometer via photonic lanterns and machine learning
    The advantage of large optical telescopes from the ground for high-contrast direct imaging relies on achieving exquisite control of the incident optical wavefront. Since the exoplanet problem almost always has a bright star within a small field of view there are usually ample photons for measuring the atmospheric and telescopedistorted wavefront. A
    Padrón-Brito, Auxiliadora et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..25P
    Citations
    0
  • Non-refereed
    Unveiling Chiron, an odd ice ball, with Webb: Ice and Gas Phases Revealed
    We present unprecedented findings on (2060) Chiron using James Webb Space Telescope (JWST) NIRSpec imaging and spectroscopy from cycle 1 GTO program 1273. Our study (Pinilla-Alonso et al. 2024 A&A Letter) marks the first detection of carbon dioxide (CO 2) and methane (CH 4) active outgassing and coma emission at heliocentric distances of ~18 au
    Pinilla-Alonso, Noemí et al.

    Advertised on:

    10
    2024
    Bibcode
    2024DPS....5640508P
    Citations
    0