Search Publications

Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster
DOI: 10.1038/s41550-024-02386-6 Bibcode: 2025NatAs...9..111P

Kaspi, Victoria M.; Smith, Kendrick M.; Güver, Tolga +26 more

The precise origins of fast radio bursts (FRBs) remain unknown. Multiwavelength observations of nearby FRB sources can provide important insights into the enigmatic FRB phenomenon. Here we present results from a sensitive, broadband X-ray and radio observational campaign of FRB 20200120E, the closest known extragalactic repeating FRB source (locat…

2025 Nature Astronomy
XMM-Newton 25
X-ray eruptions every 22 days from the nucleus of a nearby galaxy
DOI: 10.1038/s41550-023-02178-4 Bibcode: 2024NatAs...8..347G

Gendreau, Keith; van Velzen, Sjoert; Gezari, Suvi +15 more

Galactic nuclei showing recurrent phases of activity and quiescence have recently been discovered. Some have recurrence times as short as a few hours to a day and are known as quasi-periodic X-ray eruption (QPE) sources. Others have recurrence times as long as hundreds to a thousand days and are called repeating nuclear transients. Here we present…

2024 Nature Astronomy
XMM-Newton 50
Constraints on the dense matter equation of state from young and cold isolated neutron stars
DOI: 10.1038/s41550-024-02291-y Bibcode: 2024NatAs...8.1020M

Rea, N.; Marino, A.; Pons, J. A. +3 more

Neutron stars are the dense and highly magnetic relics of supernova explosions of massive stars. The quest to constrain the equation of state (EOS) of ultradense matter and thereby probe the behaviour of matter inside neutron stars is one of the core goals of modern physics and astrophysics. A promising method involves investigating the long-term …

2024 Nature Astronomy
XMM-Newton 10
X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates
DOI: 10.1038/s41550-024-02222-x Bibcode: 2024NatAs...8..596K

Güdel, M.; Koutroumpa, D.; Lisse, C. M. +3 more

Stellar winds of cool main-sequence stars are difficult to constrain observationally. One way to measure stellar mass-loss rates is to detect the soft X-ray emission from stellar astrospheres produced by charge exchange between heavy ions of the stellar wind and cold neutrals of the interstellar medium surrounding the stars. Here we report detecti…

2024 Nature Astronomy
XMM-Newton 5
The X-ray mysteries of neutron stars and white dwarfs
DOI: 10.1038/s41550-024-02430-5 Bibcode: 2024NatAs...8.1501R

Rea, Nanda; Schartel, Norbert

These two types of compact objects share several similarities, despite their different compositions. A short workshop in Spain brought communities together to share understanding of dense matter under extreme conditions.

2024 Nature Astronomy
XMM-Newton 0
Magnetar spin-down glitch clearing the way for FRB-like bursts and a pulsed radio episode
DOI: 10.1038/s41550-022-01865-y Bibcode: 2023NatAs...7..339Y

Lin, L.; Kouveliotou, C.; Baring, M. G. +16 more

Magnetars are a special subset of the isolated neutron star family, with X-ray and radio emission mainly powered by the decay of their immense magnetic fields. Many attributes of magnetars remain poorly understood: spin-down glitches or the sudden reductions in the star's angular momentum, radio bursts reminiscent of extragalactic fast radio burst…

2023 Nature Astronomy
XMM-Newton 43
A 5.3-min-period pulsing white dwarf in a binary detected from radio to X-rays
DOI: 10.1038/s41550-023-01995-x Bibcode: 2023NatAs...7..931P

Kepler, S. O.; Heywood, I.; Dhillon, V. S. +19 more

White dwarf stars are the most common stellar fossils. When in binaries, they make up the dominant form of compact object binary within the Galaxy and can offer insight into different aspects of binary formation and evolution. One of the most remarkable white dwarf binary systems identified to date is AR Scorpii (AR Sco). AR Sco is composed of an …

2023 Nature Astronomy
Gaia XMM-Newton 33
Vertical wind structure in an X-ray binary revealed by a precessing accretion disk
DOI: 10.1038/s41550-023-01929-7 Bibcode: 2023NatAs...7..715K

Fabian, A. C.; Reynolds, C. S.; Pinto, C. +11 more

The accretion of matter onto black holes and neutron stars often leads to the launching of outflows that can greatly affect the environments surrounding the compact object. An important means of studying these winds is through X-ray absorption line spectroscopy, which allows us to probe their properties along a single sightline, but usually provid…

2023 Nature Astronomy
XMM-Newton 8
A strangely light neutron star within a supernova remnant
DOI: 10.1038/s41550-022-01800-1 Bibcode: 2022NatAs...6.1444D

Doroshenko, Victor; Santangelo, Andrea; Pühlhofer, Gerd +1 more

To constrain the equation of state of cold dense matter, astrophysical measurements are essential. These are mostly based on observations of neutron stars in the X-ray band, and, more recently, also on gravitational wave observations. Of particular interest are observations of unusually heavy or light neutron stars which extend the range of centra…

2022 Nature Astronomy
Gaia XMM-Newton 180
Signatures of strong magnetization and a metal-poor atmosphere for a Neptune-sized exoplanet
DOI: 10.1038/s41550-021-01505-x Bibcode: 2022NatAs...6..141B

Mikal-Evans, Thomas; Sing, David K.; López-Morales, Mercedes +10 more

The magnetosphere of an exoplanet has yet to be unambiguously detected. Investigations of star-planet interaction and neutral atomic hydrogen absorption during transit to detect magnetic fields in hot Jupiters have been inconclusive, and interpretations of the transit absorption non-unique. In contrast, ionized species escaping a magnetized exopla…

2022 Nature Astronomy
XMM-Newton eHST 51