The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3
Artikel i vetenskaplig tidskrift, 2023

Cygnus X-3 is a high-mass X-ray binary with a compact object accreting matter from a Wolf-Rayet donor star. Recently, it has been revealed by the Imaging X-ray Polarimetry Explorer (IXPE) as a hidden Galactic ultra-luminous X-ray (ULX) source with a luminosity above the Eddington limit, along the direction of a narrow (opening angle) funnel. In between the IXPE observations, we observed Cyg X-3 with the European very long baseline interferometry (VLBI) Network at 22 GHz and the NICER X-ray instrument. To probe possible relations between the X-ray funnel and the potential radio jet from the ULX, we analysed the simultaneous multiwavelength data. Our high-resolution VLBI image reveals an elongated structure with a position angle of -3.2 ± 0.4 °, accurately perpendicular to the direction of the linear X-ray polarization. Because Cyg X-3 was in the radio quiescent state on 2022 November 10, we identify the mas-scale structure as the innermost radio jet. The finding indicates that the radio jet propagates along and within the funnel. Moreover, the jet is marginally resolved in the transverse direction. This possibly results from the strong stellar winds and the rapid orbital motion of the binary system.

X-rays: binaries

stars: jets

radio continuum: stars

stars: individual: Cygnus X-3

Författare

Jun Yang

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

Federico García

Consejo Nacional de Investigaciones Cientificas y Tecnicas

Santiago Del Palacio

University of Manchester

R. E. Spencer

Joint Institute for VLBI in Europe (JIVE)

Z. Paragi

University of Southampton

N. Castro Segura

Huazhong University of Science and Technology

Biping Gong

Shangqiu Normal University

Hong Min Cao

Yunnan Observatories

Wen Chen

Chinese Academy of Sciences

Monthly Notices of the Royal Astronomical Society: Letters

17453925 (ISSN) 17453933 (eISSN)

Vol. 526 1 L1-L7

Ämneskategorier

Astronomi, astrofysik och kosmologi

Geofysik

DOI

10.1093/mnrasl/slad111

Mer information

Senast uppdaterat

2024-01-03