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Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE
DOI: 10.1038/s41550-024-02294-9 Bibcode: 2024NatAs...8.1031V

Ingram, Adam; Kaaret, Philip; Wu, Kinwah +127 more

The accretion of matter by compact objects can be inhibited by radiation pressure if the luminosity exceeds a critical value known as the Eddington limit. The discovery of ultraluminous X-ray sources has shown that accretion can proceed even when the apparent luminosity considerably exceeds this limit. A high apparent luminosity might be produced …

2024 Nature Astronomy
INTEGRAL 48
An assessment of the association between a fast radio burst and binary neutron star merger
DOI: 10.1038/s41550-023-01917-x Bibcode: 2023NatAs...7..579M

Zhang, Bing; Moroianu, Alexandra; Wen, Linqing +4 more

Fast radio bursts (FRBs) are bright millisecond-duration radio bursts at cosmological distances. While young magnetars are the leading source candidate, recent observations suggest that there may be multiple FRB progenitor classes. Here we investigate a potential coincidence between a binary neutron star merger event, GW190425, and a bright, non-r…

2023 Nature Astronomy
INTEGRAL 47
Mapping of shadows cast on a protoplanetary disk by a close binary system
DOI: 10.1038/s41550-018-0626-6 Bibcode: 2019NatAs...3..167D

van der Plas, G.; Avenhaus, H.; Girard, J. +47 more

For a comprehensive understanding of planetary formation and evolution, we need to investigate the environment in which planets form: circumstellar disks. Here we present high-contrast imaging observations of V4046 Sagittarii, a 20-Myr-old close binary known to host a circumbinary disk. We have discovered the presence of rotating shadows in the di…

2019 Nature Astronomy
Gaia INTEGRAL 13
Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae
DOI: 10.1038/s41550-018-0505-1 Bibcode: 2018NatAs...2..731H

Hamaguchi, Kenji; Corcoran, Michael F.; Russell, Christopher M. P. +9 more

Cosmic-ray acceleration has been a long-standing mystery1,2 and, despite more than a century of study, we still do not have a complete census of acceleration mechanisms. The collision of strong stellar winds in massive binary systems creates powerful shocks that have been expected to produce high-energy cosmic rays through Fermi acceler…

2018 Nature Astronomy
INTEGRAL XMM-Newton 47
An elevation of 0.1 light-seconds for the optical jet base in an accreting Galactic black hole system
DOI: 10.1038/s41550-017-0273-3 Bibcode: 2017NatAs...1..859G

Harrison, F. A.; Stern, D.; Altamirano, D. +25 more

Relativistic plasma jets are observed in many systems that host accreting black holes. According to theory, coiled magnetic fields close to the black hole accelerate and collimate the plasma, leading to a jet being launched1-3. Isolating emission from this acceleration and collimation zone is key to measuring its size and understanding …

2017 Nature Astronomy
INTEGRAL 82
Gamma-ray observatory INTEGRAL reloaded
DOI: 10.1038/s41550-017-0083 Bibcode: 2017NatAs...1E..83V

van den Heuvel, Edward P. J.

The scientific aims of the European Space Agency's International Gamma-Ray Astrophysics Laboratory are considerably extended because of its unique capability to identify electromagnetic counterparts to sources of gravitational waves and ultra-high-energy neutrinos.

2017 Nature Astronomy
INTEGRAL 4