A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Observations of a radio-bright, X-ray obscured GRS 1915+105
Tekijät: Motta SE, Kajava JJE, Giustini M, Williams DRA, Del Santo M, Fender R, Green DA, Heywood I, Rhodes L, Segreto A, Sivakoff G, Woudt PA
Kustantaja: OXFORD UNIV PRESS
Julkaisuvuosi: 2021
Journal: Monthly Notices of the Royal Astronomical Society
Tietokannassa oleva lehden nimi: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Lehden akronyymi: MON NOT R ASTRON SOC
Vuosikerta: 503
Numero: 1
Aloitussivu: 152
Lopetussivu: 161
Sivujen määrä: 10
ISSN: 0035-8711
DOI: https://doi.org/10.1093/mnras/stab511
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/58640383
The Galactic black hole transient GRS 1915+105 is famous for its markedly variable X-ray and radio behaviour, and for being the archetypal galactic source of relativistic jets. It entered an X-ray outburst in 1992 and has been active ever since. Since 2018 GRS 1915+105 has declined into an extended low-flux X-ray plateau, occasionally interrupted by multiwavelength flares. Here, we report the radio and X-ray properties of GRS 1915+105 collected in this new phase, and compare the recent data to historic observations. We find that while the X-ray emission remained unprecedentedly low for most of the time following the decline in 2018, the radio emission shows a clear mode change half way through the extended X-ray plateau in 2019 June: from low flux (similar to 3mJy) and limited variability, to marked flaring with fluxes two orders of magnitude larger. GRS 1915+105 appears to have entered a low-luminosity canonical hard state, and then transitioned to an unusual accretion phase, characterized by heavy X-ray absorption/obscuration. Hence, we argue that a local absorber hides from the observer the accretion processes feeding the variable jet responsible for the radio flaring. The radio-X-ray correlation suggests that the current low X-ray flux state may be a signature of a super-Eddington state akin to the X-ray binaries SS433 or V404 Cyg.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
