Swift-XRT location of the ongoing Terzan 5 outburst

Bibcode
2010ATel.2920....1L
Linares, M.; Altamirano, D.
Bibliographical reference

The Astronomer's Telegram, #2920

Advertised on:
10
2010
Number of authors
2
IAC number of authors
0
Citations
3
Refereed citations
2
Description
IBIS-ISGRI observations on 2010-10-10 (Bordas et al. ATel #2919) as well as RXTE-PCA scans on 2010-10-09 (http://lheawww.gsfc.nasa.gov/users/craigm/galscan/html/EXO_1745-248.html) showed enhanced X-ray emission from the direction of the globular cluster Terzan 5. We analysed a ~500 s Swift-XRT observation of the field starting on 2010-10-10 01:32:05 UT, detecting one bright source at a position of RA=267.021 DEC=-24.781 (J2000; 3.6 arc-seconds error radius), consistent with Terzan 5 and about 5.3 arc-seconds from the Chandra location of the neutron star transient EXO 1745-248 (Heinke et al.
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