The Eclipsing X-ray Burster in Terzan 5 is Probably Not the 2000 Transient

Bibcode
2010ATel.2933....1H
Heinke, C. O.; Linares, M.; Gladstone, J.; Homan, J.; Altamirano, D.; Pooley, D.
Bibliographical reference

The Astronomer's Telegram, #2933

Advertised on:
10
2010
Number of authors
6
IAC number of authors
0
Citations
6
Refereed citations
5
Description
The transient LMXB and 11 Hz pulsar currently in outburst in Terzan 5 (ATEL #2919, #2920, #2922, #2924, #2932) has been recently observed to show at least one eclipse of 511 s duration (ATEL #2929). We have checked the Chandra lightcurves (readout streak and dust-scattered halo) from the 2000 July 24 observation (Heinke et al. 2003, ApJ, 590, 809), and find no eclipses in the 45 ks (12.5 hour) observation.
Type
Non-refereed

It may interest you

  • Non-refereed
    RAD@home Citizen Scientists Uncover Emerging Jet-Galaxy Interactions
    The RAD12 object's recent investigation (Hota et al. 2022), via the RAD@home Astronomy Collaboratory, has provided a streamlined and focused perspective on the complex subject of jet-galaxy interactions, which has always posed a significant challenge for observational confirmation. This emerging field holds increasing significance, providing a
    Hota, Ananda et al.

    Advertised on:

    1
    2024
    Bibcode
    2024asi..confP..76H
    Citations
    0
  • Non-refereed
    A Disc Wind Where You Least Expect It: The Outflow in the Short-period X-ray Binary UW CrB
    Studying outflows of low mass X-ray binaries (LMXBs) is important for understanding the physics of accretion, the evolution of compact binaries, and dynamics of the local interstellar medium. One significant source of these outflows is the accretion disc wind, which can blow away vast amounts of material from the disc before it can be accreted on
    Fijma, Stefanie et al.

    Advertised on:

    5
    2024
    Bibcode
    2024HEAD...2150106F
    Citations
    0
  • Non-refereed
    Constraining the core-rotation rate along the red-giant evolution
    The evolution of the core rotation rate of red giant stars is a key parameter in understanding the stellar behavior in the late phases of stellar evolution. Thanks to the mixed-dipole modes, we can constrain the core rotation and internal rotational gradient as a star advances through the red-giant phase. This master thesis presents a pipeline
    Muntean, N. et al.

    Advertised on:

    3
    2024
    Bibcode
    2024aecc.conf...34M
    Citations
    0