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Perspectives of the LOBSTER-EYE monitor in the soft X-ray observing the Galactic center region

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00560479" target="_blank" >RIV/67985815:_____/22:00560479 - isvavai.cz</a>

  • Alternative codes found

    RIV/68407700:21230/22:00359281

  • Result on the web

    <a href="https://doi.org/10.1016/j.jheap.2022.06.001" target="_blank" >https://doi.org/10.1016/j.jheap.2022.06.001</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.jheap.2022.06.001" target="_blank" >10.1016/j.jheap.2022.06.001</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Perspectives of the LOBSTER-EYE monitor in the soft X-ray observing the Galactic center region

  • Original language description

    We show the lobster-eye (LE) monitor's perspectives and observing plan based on a small LE telescope on a small (CubeSat-like) satellite platform. This instrument is important because it is able to provide wide-field X-ray imaging. We present the possibilities of monitoring the Galactic center region in the soft X-ray energy band. The reason is that many X-ray binaries, especially those with a low-mass lobe filling secondary and mostly the neutron star accretor, concentrate in the bulge surrounding the center of our Galaxy. Several such binaries are expected to be present in our monitor's field of view (a square of about 5 x 5 degrees). We show the long-term activity of the examples of X-ray binaries located in this region. We present the typical features of such objects' long-term X-ray activity (e.g., outbursts and state transitions) and discuss how the lobster-eye monitor can contribute. Observing in the soft X-ray band is the most promising because their X-ray intensity is the highest in this band. (C) 2022 Elsevier B.V. All rights reserved.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10306 - Optics (including laser optics and quantum optics)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Journal of High Energy Astrophysics

  • ISSN

    2214-4048

  • e-ISSN

    2214-4056

  • Volume of the periodical

    35

  • Issue of the periodical within the volume

    August

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    8

  • Pages from-to

    69-76

  • UT code for WoS article

    000835727800004

  • EID of the result in the Scopus database