Search Publications

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
A temperate super-Jupiter imaged with JWST in the mid-infrared
DOI: 10.1038/s41586-024-07837-8 Bibcode: 2024Natur.633..789M

Henning, Th.; Morley, C. V.; Lagrange, A. -M. +16 more

Of the approximately 25 directly imaged planets to date, all are younger than 500 Myr, and all but six are younger than 100 Myr (ref. 1). Eps Ind A (HD209100, HIP108870) is a K5V star of roughly solar age (recently derived as 3.7–5.7 Gyr (ref. 2) and 3.5

2024 Nature
Gaia JWST 17
Molecular Outflow in the Reionization-epoch Quasar J2054-0005 Revealed by OH 119 µm Observations
DOI: 10.3847/1538-4357/ad0df5 Bibcode: 2024ApJ...962....1S

Fujimoto, Seiji; Inoue, Akio K.; Hashimoto, Takuya +8 more

Molecular outflows are expected to play a key role in galaxy evolution at high redshift. To study the impact of outflows on star formation at the epoch of reionization, we performed sensitive Atacama Large Millimeter/submillimeter Array observations of OH 119 µm toward J2054-0005, a luminous quasar at z = 6.04. The OH line is detected and ex…

2024 The Astrophysical Journal
Herschel 17
The ALMA-CRISTAL survey: Discovery of a 15 kpc-long gas plume in a z = 4.54 Lyman-α blob
DOI: 10.1051/0004-6361/202449192 Bibcode: 2024A&A...689A.145S

Lutz, D.; Förster Schreiber, N. M.; Veilleux, S. +25 more

Massive star-forming galaxies in the high-redshift universe host large reservoirs of cold gas in their circumgalactic medium (CGM). Traditionally, these reservoirs have been linked to diffuse H I Lyman-α (Lyα) emission extending beyond ≈10 kpc scales. In recent years, millimeter and submillimeter observations have started to identify even colder g…

2024 Astronomy and Astrophysics
Gaia eHST 17
Taking the Milky Way for a spin: disc formation in the ARTEMIS simulations
DOI: 10.1093/mnras/stad3369 Bibcode: 2024MNRAS.527.7070D

Belokurov, Vasily; Dillamore, Adam M.; Font, Andreea S. +1 more

We investigate the formation (spin-up) of galactic discs in the ARTEMIS simulations of Milky Way (MW)-mass galaxies. In almost all galaxies, discs spin up at higher [Fe/H] than the MW. Those galaxies that contain an analogue of the Gaia Sausage-Enceladus (GSE) spin up at a lower average metallicity than those without. We identify six galaxies with…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 17
Detection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer
DOI: 10.3847/1538-4357/ad1ce4 Bibcode: 2024ApJ...963....5E

Ingram, Adam; Kaaret, Philip; Wu, Kinwah +142 more

Observations of linear polarization in the 2–8 keV energy range with the Imaging X-ray Polarimetry Explorer (IXPE) explore the magnetic field geometry and dynamics of the regions generating nonthermal radiation in relativistic jets of blazars. These jets, particularly in blazars whose spectral energy distribution peaks at X-ray energies, emit X-ra…

2024 The Astrophysical Journal
XMM-Newton 17
Supermassive black hole mass in the massive elliptical galaxy M87 from integral-field stellar dynamics using OASIS and MUSE with adaptive optics: assessing systematic uncertainties
DOI: 10.1093/mnras/stad3309 Bibcode: 2024MNRAS.527.2341S

Cappellari, Michele; Hartke, Johanna; Simon, David A.

The massive elliptical galaxy M87 has been the subject of several supermassive black hole mass measurements from stellar dynamics, gas dynamics, and recently the black hole shadow by the Event Horizon Telescope. This uniquely positions M87 as a benchmark for alternative black hole mass determination methods. Here, we use stellar kinematics extract…

2024 Monthly Notices of the Royal Astronomical Society
eHST 17
A Comprehensive Investigation of Metals in the Circumgalactic Medium of Nearby Dwarf Galaxies
DOI: 10.3847/1538-4357/acfe6b Bibcode: 2024ApJ...960...55Z

McQuinn, Kristen B. W.; Burchett, Joseph N.; Putman, Mary E. +7 more

Dwarf galaxies are found to have lost most of their metals via feedback processes; however, there still lacks consistent assessment on the retention rate of metals in their circumgalactic medium (CGM). Here we investigate the metal content in the CGM of 45 isolated dwarf galaxies with M * = 106.5-9.5 M (M 20…

2024 The Astrophysical Journal
eHST 17
TIPSY: Trajectory of Infalling Particles in Streamers around Young stars. Dynamical analysis of the streamers around S CrA and HL Tau
DOI: 10.1051/0004-6361/202348007 Bibcode: 2024A&A...683A.133G

Yen, Hsi-Wei; Williams, Jonathan P.; Birnstiel, Til +3 more

Context. Elongated trails of infalling gas, often referred to as "streamers," have recently been observed around young stellar objects (YSOs) at different evolutionary stages. This asymmetric infall of material can significantly alter star and planet formation processes, especially in the more evolved YSOs.
Aims: In order to ascertain the inf…

2024 Astronomy and Astrophysics
Gaia 17
Properties of an Interplanetary Shock Observed at 0.07 and 0.7 au by Parker Solar Probe and Solar Orbiter
DOI: 10.3847/1538-4357/ad187d Bibcode: 2024ApJ...962..147T

Zank, Gary P.; Zhao, Lingling; Karlsson, Tomas +23 more

The Parker Solar Probe (PSP) and Solar Orbiter (SolO) missions opened a new observational window in the inner heliosphere, which is finally accessible to direct measurements. On 2022 September 5, a coronal mass ejection (CME)-driven interplanetary (IP) shock was observed as close as 0.07 au by PSP. The CME then reached SolO, which was radially wel…

2024 The Astrophysical Journal
SolarOrbiter 17