Search Publications

The SRG/eROSITA all-sky survey. First X-ray catalogues and data release of the western Galactic hemisphere
DOI: 10.1051/0004-6361/202347165 Bibcode: 2024A&A...682A..34M

Zhang, X.; Haberl, F.; Burwitz, V. +142 more

The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying the sky in December 2019, with the aim of producing all-sky X-ray source lists and sky maps of an unprecedented depth. Here we present catalogues of both point-like and extended sources using the data acquired in the first six months of survey operations…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 197
The more the merrier: SRG/eROSITA discovers two further galaxies showing X-ray quasi-periodic eruptions
DOI: 10.1051/0004-6361/202348881 Bibcode: 2024A&A...684A..64A

Gromadzki, M.; Salvato, M.; Liu, Z. +20 more

X-ray quasi-periodic eruptions (QPEs) are a novel addition to the group of extragalactic transients. With only a select number of known sources, and many more models published trying to explain them, we are so far limited in our understanding by small number statistics. In this work, we report the discovery of two further galaxies showing QPEs, he…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 48
1100 days in the life of the supernova 2018ibb. The best pair-instability supernova candidate, to date
DOI: 10.1051/0004-6361/202346855 Bibcode: 2024A&A...683A.223S

Filippenko, Alexei V.; Fransson, Claes; Gromadzki, Mariusz +63 more

Stars with zero-age main sequence masses between 140 and 260 M are thought to explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can produce up to several tens of solar masses of radioactive nickel, resulting in luminous transients similar to some superluminous supernovae (SLSNe). Yet, no unambigu…

2024 Astronomy and Astrophysics
Gaia XMM-Newton eHST 36
Magnetic field properties inside the jet of Mrk 421. Multiwavelength polarimetry, including the Imaging X-ray Polarimetry Explorer
DOI: 10.1051/0004-6361/202347408 Bibcode: 2024A&A...681A..12K

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +133 more


Aims: We aim to probe the magnetic field geometry and particle acceleration mechanism in the relativistic jets of supermassive black holes.
Methods: We conducted a polarimetry campaign from radio to X-ray wavelengths of the high-synchrotron-peak (HSP) blazar Mrk 421, including Imaging X-ray Polarimetry Explorer (IXPE) measurements from 2…

2024 Astronomy and Astrophysics
XMM-Newton 26
Discovery of a strong rotation of the X-ray polarization angle in the galactic burster GX 13+1
DOI: 10.1051/0004-6361/202449318 Bibcode: 2024A&A...688A.170B

Done, Chris; Kaaret, Philip; Wu, Kinwah +106 more

Weakly magnetized neutron stars in X-ray binaries show a complex phenomenology with several spectral components that can be associated with the accretion disk, the boundary, and/or a spreading layer, a corona, and a wind. Spectroscopic information alone, however, is not enough to distinguish these components. The analysis of the timing data reveal…

2024 Astronomy and Astrophysics
XMM-Newton 17
2D disc modelling of the JWST line spectrum of EX Lupi
DOI: 10.1051/0004-6361/202347730 Bibcode: 2024A&A...683A.219W

Woitke, P.; Kamp, I.; Ábrahám, P. +3 more

We introduce a number of improvements to the thermo-chemical disc modelling code PRODIMO and new theoretical approaches that can be used to better predict and analyse the JWST line spectra of protoplanetary discs. We developed a new line escape probability method for disc geometries, and a new scheme for dust settling, and discuss how to apply UV …

2024 Astronomy and Astrophysics
Herschel XMM-Newton 17
AGNs in massive galaxy clusters: Role of galaxy merging, infalling groups, cluster mass, and dynamical state
DOI: 10.1051/0004-6361/202348212 Bibcode: 2024A&A...684A.111K

Koulouridis, E.; Drigga, E.; Gkini, A.

Context. There is compelling evidence that active galactic nuclei (AGNs) in high-density regions have undergone a different evolution than their counterparts in the field, indicating that they are strongly affected by their environment. However, we still lack a comprehensive understanding of the dominant mechanisms that trigger the nucleus and the…

2024 Astronomy and Astrophysics
XMM-Newton eHST 17
Binarity at LOw Metallicity (BLOeM): A spectroscopic VLT monitoring survey of massive stars in the SMC
DOI: 10.1051/0004-6361/202451586 Bibcode: 2024A&A...690A.289S

van Loon, J. Th.; Wang, C.; Crowther, P. A. +75 more

Surveys in the Milky Way and Large Magellanic Cloud have revealed that the majority of massive stars will interact with companions during their lives. However, knowledge of the binary properties of massive stars at low metallicity, and therefore in conditions approaching those of the Early Universe, remain sparse. We present the Binarity at LOw Me…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 17
Ticking away: The long-term X-ray timing and spectral evolution of eRO-QPE2
DOI: 10.1051/0004-6361/202451218 Bibcode: 2024A&A...690A..80A

Merloni, A.; Ponti, G.; Miniutti, G. +11 more

Quasi-periodic eruptions (QPEs) are repeated X-ray flares from galactic nuclei that recur every few hours to days, depending on the source. Despite some diversity in the recurrence and amplitude of eruptions, their striking regularity has motivated theorists to associate QPEs with orbital systems. Among the known QPE sources, eRO-QPE2 has shown th…

2024 Astronomy and Astrophysics
XMM-Newton 17
The SRG/eROSITA All-Sky Survey. SRG/eROSITA cross-calibration with Chandra and XMM-Newton using galaxy cluster gas temperatures
DOI: 10.1051/0004-6361/202349006 Bibcode: 2024A&A...688A.107M

Zhang, X.; Pacaud, F.; Ramos-Ceja, M. E. +17 more

Galaxy cluster gas temperatures (T) play a crucial role in many cosmological and astrophysical studies. However, it has been shown that T measurements can significantly vary between different X-ray telescopes. These T biases can propagate to several cluster applications in which T can be used, such as measuring hydrostatic cluster masses and const…

2024 Astronomy and Astrophysics
XMM-Newton 16