The Transition from Outburst to Low Level Activity in the Low-Mass X-Ray Binary SAX J1747.0-2853

Bibcode
2004BaltA..13..163W
Werner, N.; in't Zand, J. J. M.; Natalucci, L.; Markwardt, C. B.; Cornelisse, R.; Bazzano, A.; Cocchi, M.; Heise, J.; Ubertini, P.
Bibliographical reference

Baltic Astronomy, Vol. 13, p. 163-166

Advertised on:
0
2004
Number of authors
9
IAC number of authors
0
Citations
1
Refereed citations
0
Description
SAX J1747.0-2853 is an X-ray transient which exhibited several outbursts between 1998 and 2001 and most probably in 1976. The outburst of 2000 was the longest and brightest. We have analyzed X-ray data sets that focus on times around the 2000 outburst and were obtained with l BeppoSAX, XMM-Newton and l RXTE.
Type
Refereed

It may interest you

  • Refereed
    The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
    WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2-deg field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU
    Jin, Shoko et al.

    Advertised on:

    5
    2024
    Bibcode
    2024MNRAS.530.2688J
    Citations
    33
  • Refereed
    The extent and power of 'maintenance mode' feedback in MaNGA AGN
    We study the ionized gas kinematics of 293 Active Galactic Nucleus (AGN) hosts as compared to that of 485 control galaxies from the MaNGA-SDSS survey using measurements of the [O III]$\lambda$5007 Å emission-line profiles, presenting flux, velocity, and W$_{80}$ maps. In 45 per cent of the AGN, a broad component was needed to fit the line profiles
    Gatto, Lara et al.

    Advertised on:

    5
    2024
    Bibcode
    2024MNRAS.530.3059G
    Citations
    0
  • Refereed
    TOI-663: A newly discovered multi-planet system with three transiting mini-Neptunes orbiting an early M star
    We present the detection of three exoplanets orbiting the early M dwarf TOI-663 (TIC 54962195; V = 13.7 mag, J = 10.4 mag, R ★ = 0.512 ± 0.015 R ⊙, M ★ = 0.514 ± 0.012 M ⊙, d = 64 pc). TOI-663 b, c, and d, with respective radii of 2.27 ± 0.10 R ⊕, 2.26 ± 0.10 R ⊕, and 1.92 ± 0.13 R ⊕ and masses of 4.45 ± 0.65 M ⊕, 3.65 ± 0.97 M ⊕, and <5.2 M ⊕ at
    Cointepas, M. et al.

    Advertised on:

    5
    2024
    Bibcode
    2024A&A...685A..19C
    Citations
    0