Search Publications

Confronting sparse Gaia DR3 photometry with TESS for a sample of around 60 000 OBAF-type pulsators
DOI: 10.1051/0004-6361/202450489 Bibcode: 2024A&A...688A..93H

Aerts, Conny; Hey, Daniel

Context. The Gaia mission has delivered hundreds of thousands of variable star light curves in multiple wavelengths. Recent work demonstrates that these light curves can be used to identify (non-)radial pulsations in OBAF-type stars, despite their irregular cadence and low light curve precision, of the order of a few millimagnitudes. With the cons…

2024 Astronomy and Astrophysics
Gaia 19
Alive but Barely Kicking: News from 3+ yr of Swift and XMM-Newton X-Ray Monitoring of Quasiperiodic Eruptions from eRO-QPE1
DOI: 10.3847/2041-8213/ad2a5c Bibcode: 2024ApJ...963L..47P

Altamirano, D.; Wevers, T.; Karas, V. +11 more

Quasiperiodic eruptions (QPEs) represent a novel class of extragalactic X-ray transients that are known to repeat at roughly regular intervals of a few hours to days. Their underlying physical mechanism is a topic of heated debate, with most models proposing that they originate either from instabilities within the inner accretion flow or from orbi…

2024 The Astrophysical Journal
XMM-Newton 19
The 33 M black hole Gaia BH3 is part of the disrupted ED-2 star cluster
DOI: 10.1051/0004-6361/202450425 Bibcode: 2024A&A...687L...3B

Mazeh, T.; Caffau, E.; Cabrera-Ziri, I. +19 more

Context. The Gaia Collaboration has recently reported the detection of a 33 M black hole in a wide binary system located in the solar neighbourhood.
Aims: Here we explore the relationship between this black hole, known as Gaia BH3, and the nearby ED-2 halo stellar stream.
Methods: We studied the orbital characteristics of the…

2024 Astronomy and Astrophysics
Gaia 19
The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields
DOI: 10.1051/0004-6361/202346730 Bibcode: 2024A&A...686A.170W

Hoekstra, Henk; Sifón, Cristóbal; Heymans, Catherine +51 more

We present the final data release of the Kilo-Degree Survey (KiDS-DR5), a public European Southern Observatory (ESO) wide-field imaging survey optimised for weak gravitational lensing studies. We combined matched-depth multi-wavelength observations from the VLT Survey Telescope and the VISTA Kilo-degree INfrared Galaxy (VIKING) survey to create a …

2024 Astronomy and Astrophysics
Gaia 19
Cosmic hide and seek: The volumetric rate of X-ray quasi-periodic eruptions
DOI: 10.1051/0004-6361/202348949 Bibcode: 2024A&A...684L..14A

Salvato, M.; Liu, Z.; Buchner, J. +6 more

Multiwavelength extragalactic nuclear transients, particularly those detectable as multi-messengers, are among the primary drivers for the next-generation observatories. X-ray quasi-periodic eruptions (QPEs) are the most recent and perhaps most peculiar addition to this group. Here, we report a first estimate of the volumetric rate of QPEs based o…

2024 Astronomy and Astrophysics
Gaia 19
Hydrogen sulfide and metal-enriched atmosphere for a Jupiter-mass exoplanet
DOI: 10.1038/s41586-024-07760-y Bibcode: 2024Natur.632..752F

Deming, Drake; Sing, David K.; Fu, Guangwei +15 more

As the closest transiting hot Jupiter to Earth, HD 189733b has been the benchmark planet for atmospheric characterization1–3. It has also been the anchor point for much of our theoretical understanding of exoplanet atmospheres from composition4, chemistry5,6, aerosols7 to atmospheric dynamics8

2024 Nature
JWST 19
JWST Directly Images Giant Planet Candidates Around Two Metal-polluted White Dwarf Stars
DOI: 10.3847/2041-8213/ad2348 Bibcode: 2024ApJ...962L..32M

Barclay, Thomas; Hermes, J. J.; Reach, William T. +9 more

We report the discovery of two directly imaged, giant planet candidates orbiting the metal-rich, hydrogen atmosphere white dwarfs WD 1202‑232 and WD 2105‑82. JWST's Mid-Infrared Instrument (MIRI) data on these two stars show a nearby resolved source at a projected separation of 11.47 and 34.62 au, respectively. Assuming the planets formed at the s…

2024 The Astrophysical Journal
Gaia JWST 19
The ALMA Reionization Era Bright Emission Line Survey: The molecular gas content of galaxies at z 7
DOI: 10.1051/0004-6361/202347281 Bibcode: 2024A&A...682A..24A

Inami, H.; De Looze, I.; Schneider, R. +19 more

A key to understanding the formation of the first galaxies is to quantify the content of the molecular gas as the fuel for star formation activity through the epoch of reionization. In this paper, we use the 158µm [C II] fine-structure emission line as a tracer of the molecular gas in the interstellar medium (ISM) in a sample of 𝓏 = 6.5-7.5 galaxi…

2024 Astronomy and Astrophysics
eHST 19
JWST Imaging of Edge-on Protoplanetary Disks. I. Fully Vertically Mixed 10 µm Grains in the Outer Regions of a 1000 au Disk
DOI: 10.3847/1538-3881/acf9a7 Bibcode: 2024AJ....167...77D

Duchêne, Gaspard; Wolff, Schuyler G.; Perrin, Marshall D. +6 more

Scattered light imaging of protoplanetary disks provides key insights on the geometry and dust properties in the disk surface. Here, we present James Webb Space Telescope (JWST) 2–21 µm images of a 1000 au radius edge-on protoplanetary disk surrounding an 0.4 M young star in Taurus, Two Micron All Sky Survey (2MASS) J04202144 + …

2024 The Astronomical Journal
Herschel eHST JWST 19
JWST detection of extremely excited outflowing CO and H2O in VV 114 E SW: A possible rapidly accreting IMBH
DOI: 10.1051/0004-6361/202348469 Bibcode: 2024A&A...682A.182G

González-Alfonso, Eduardo; Pereira-Santaella, Miguel; Neufeld, David A. +3 more

Mid-infrared (mid-IR) gas-phase molecular bands are powerful diagnostics of the warm interstellar medium. We report the James Webb Space Telescope detection of the CO v = 1 − 0 (4.4 − 5.0 µm) and H2O ν2 = 1 − 0 (5.0 − 7.8 µm) ro-vibrational bands, both in absorption, toward the "s2" core in the southwest nucleus o…

2024 Astronomy and Astrophysics
JWST 19