4U 1608-52 is back to quiescence after its 2007-2009 outburst

Bibcode
2009ATel.2264....1L
Linares, M.; Altamirano, D.; Degenaar, N.; Wijnands, R.
Referencia bibliográfica

The Astronomer's Telegram, #2264

Fecha de publicación:
10
2009
Número de autores
4
Número de autores del IAC
0
Número de citas
2
Número de citas referidas
2
Descripción
After an outburst that lasted more than 2.3 years (starting around June 12th., 2007; Palmer et al., ATel #1113), the neutron star transient and atoll source 4U 1608-52 has returned to quiescence. The source was last detected by Swift-BAT, RXTE-PCA and RXTE-ASM on September 14th. (~0.006 BAT c/s/cm2), September 19th. (~3.5 mCrab) and October 5th. (~1.4 ASM c/s), 2009, respectively. We obtained daily Swift-XRT observations since October 20th.
Tipo
Sin árbitro
Estrellas de neutrones

Te puede interesar

  • Sin árbitro
    Conceptual design of the infrared integral field spectropolarimeter for the European Solar Telescope
    The European Solar Telescope (EST) will be Europe's most ambitious ground-based infrastructure in solar physics. It will have a primary mirror with a diameter of 4.2m, which will make it the largest in Europe, and of identical aperture as the largest solar telescope available worldwide, namely the Daniel K. Inouye Telescope (DKIST) installed at the
    Quintero Noda, C. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..2CQ
    Número de citas
    0
  • Sin árbitro
    Detector upgrade in EMIR@GTC: on-sky performances
    EMIR was shipped to the GTC on May 2016 and had its first light on June 2016. Since the beginning, the EMIR performances have been severely hampered by the many instabilities in the infrared detector, a 2048x2048 Hawaii2, built with the old original technology of the Teledyne Hawaii series. Despite of this, the instrument has proven to be powerful
    Garzón, Francisco et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..27G
    Número de citas
    0
  • Sin árbitro
    The Large Interferometer For Exoplanets (LIFE): a space mission for mid-infrared nulling interferometry
    The Large Interferometer For Exoplanets (LIFE) is a proposed space mission that enables the spectral characterization of the thermal emission of exoplanets in the solar neighborhood. The mission is designed to search for global atmospheric biosignatures on dozens of temperate terrestrial exoplanets and it will naturally investigate the diversity of
    Glauser, Adrian M. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13095E..1DG
    Número de citas
    0