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Fragments of harmony amid apparent chaos: A closer look at the X-ray quasi-periodic eruptions of the galaxy RX J1301.9+2747
DOI: 10.1051/0004-6361/202450861 Bibcode: 2024A&A...692A..15G

Alexander, Kate D.; Miniutti, Giovanni; Kara, Erin +17 more

Quasi-periodic eruptions (QPEs) are an extreme X-ray variability phenomenon associated with low-mass (MBH < 107 M) supermassive black holes (SMBHs). First discovered in the nucleus of the galaxy GSN 069, they have been so far securely detected in five other galaxies, including RX J1301.9+2747. When detected, th…

2024 Astronomy and Astrophysics
Exosat XMM-Newton 11
XMM-Newton - NuSTAR monitoring campaign of the Seyfert 1 galaxy IC 4329A
DOI: 10.1051/0004-6361/202348760 Bibcode: 2024A&A...687A..51T

Paltani, S.; Tombesi, F.; Privon, G. C. +13 more

We present the results of a joint XMM-Newton and NuSTAR campaign on the active galactic nucleus (AGN) IC 4329A, consisting of 9 × 20 ks XMM-Newton observations, and 5 × 20 ks NuSTAR observations within nine days, performed in August 2021. Within each observation, the AGN is not very variable, and the fractional variability never exceeds 5%. Flux v…

2024 Astronomy and Astrophysics
Exosat XMM-Newton 3
High-resolution spectroscopy of the intermediate polar EX Hydrae. II. The inner disk radius
DOI: 10.1051/0004-6361/202244473 Bibcode: 2024A&A...686A.304B

Beuermann, K.; Reinsch, K.

EX Hya is one of the best studied, but still enigmatic intermediate polars. We present phase-resolved blue VLT/UVES high-resolution (λ/Δλ ≃ 16.000) spectra of EX Hya taken in January 2004. Our analysis involves a unique decomposition of the Balmer line profiles into the spin-modulated line wings that represent…

2024 Astronomy and Astrophysics
Exosat 1
ExoplANETS-A: A virtual observatory database for host stars and planetary systems. The effect of XUV on planet atmospheres
DOI: 10.1051/0004-6361/202449832 Bibcode: 2024A&A...688A..45M

Huélamo, N.; García, R. A.; Solano, E. +12 more

Context. ExoplANETS-A is an EU Horizon-2020 project with the primary objective of establishing new knowledge on exoplanet atmospheres. Intimately related to this topic is the study of the host stars' radiative properties in order to understand the environment in which exoplanets lie.
Aims: The aim of this work is to exploit archived data from…

2024 Astronomy and Astrophysics
Exosat Gaia XMM-Newton eHST 0
Current and secular accretion rates of EX Hydrae
DOI: 10.1051/0004-6361/202450486 Bibcode: 2024A&A...687A.273B

Beuermann, K.; Reinsch, K.

We report an observed accretion rate of Ṁ1 = (3.86 ± 0.60) × 10−11 M yr−1 for the white dwarf in the short-period, intermediate polar EX Hya. This result is based upon the accretion-induced 4π-averaged energy flux from 2.45 µm to 100 keV and the corresponding luminosity at the G…

2024 Astronomy and Astrophysics
Exosat Gaia IUE 0