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Outburst and flares from the unique source SWIFT J1955+2614

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F12%3A00201044" target="_blank" >RIV/68407700:21230/12:00201044 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/12:00388611

  • Result on the web

    <a href="http://dx.doi.org/10.1111/j.1365-2966.2012.20668.x" target="_blank" >http://dx.doi.org/10.1111/j.1365-2966.2012.20668.x</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1111/j.1365-2966.2012.20668.x" target="_blank" >10.1111/j.1365-2966.2012.20668.x</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Outburst and flares from the unique source SWIFT J1955+2614

  • Original language description

    We present results of our analysis of the optical emission of the unique source GRB 070610/SWIFT J195509+261406 during its 2007 outburst and discuss the implications of the non-detection of the very faint optical counterpart in quiescence. We analyse thestatistical properties of the optical brightness and X-ray intensity during the outburst and determined an approximate value of the mean colour index R-I. The optical emission has the form of spikes whose duration decreases with the outburst's progress,and the spectral energy distribution from the X-ray to the optical bands undergoes variations during the spikes. We show that the optical emission can be explained by a synchrotron mechanism while any thermal component is below the detection limit. We discuss the similarities between synchrotron emission of J1955 and the optical afterglows (OAs) of the extragalactic long gamma-ray bursts. We conclude that while the emission mechanisms in J1955 and OAs are quite similar, the configuratio

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2012

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    0035-8711

  • e-ISSN

  • Volume of the periodical

    422

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    9

  • Pages from-to

    981-989

  • UT code for WoS article

    000303912800005

  • EID of the result in the Scopus database