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Gaia Data Release 3. Stellar chromospheric activity and mass accretion from Ca II IRT observed by the Radial Velocity Spectrometer
DOI: 10.1051/0004-6361/202244156 Bibcode: 2023A&A...674A..30L

Hatzidimitriou, D.; Marshall, D. J.; Andretta, V. +82 more

Context. The Gaia Radial Velocity Spectrometer (RVS) provides the unique opportunity of a spectroscopic analysis of millions of stars at medium resolution (λ/Δλ ∼ 11 500) in the near-infrared (845−872 nm). This wavelength range includes the Ca II infrared triplet (IRT) at 850.03, 854.44, and 866.45 nm, which is a good indicator of magnetic activit…

2023 Astronomy and Astrophysics
Gaia 19
A shared accretion instability for black holes and neutron stars
DOI: 10.1038/s41586-022-05648-3 Bibcode: 2023Natur.615...45V

Altamirano, D.; Belloni, T.; Degenaar, N. +20 more

Accretion disks around compact objects are expected to enter an unstable phase at high luminosity1. One instability may occur when the radiation pressure generated by accretion modifies the disk viscosity, resulting in the cyclic depletion and refilling of the inner disk on short timescales2. Such a scenario, however, has onl…

2023 Nature
eHST 19
ODIN: Where Do Lyα Blobs Live? Contextualizing Blob Environments within Large-scale Structure
DOI: 10.3847/1538-4357/acd341 Bibcode: 2023ApJ...951..119R

Dey, Arjun; Gronwall, Caryl; Jeong, Woong-Seob +16 more

While many Lyα blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5352 Lyα emitters (LAEs) and 129 LABs at z = 3.1 identified over a ~9.5 deg2 area in early data from the ongoing One-hundred-deg

2023 The Astrophysical Journal
Gaia 19
RASS-MCMF: a full-sky X-ray selected galaxy cluster catalogue
DOI: 10.1093/mnras/stad2729 Bibcode: 2023MNRAS.526.3757K

Klein, Matthias; Hernández-Lang, Daniel; Mohr, Joseph J. +2 more

We present the RASS-MCMF catalogue of 8449 X-ray selected galaxy clusters over 25 000 deg2 of extragalactic sky. The accumulation of deep multiband optical imaging data, the development of the Multi-Component Matched Filter (MCMF) cluster confirmation algorithm, and the release of the DESI Legacy Survey DR10 catalogue makes it possible …

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19
Production of 44Ti and Iron-group Nuclei in the Ejecta of 3D Neutrino-driven Supernovae
DOI: 10.3847/2041-8213/ad045b Bibcode: 2023ApJ...957L..25S

Sieverding, Andre; Kresse, Daniel; Janka, Hans-Thomas

The radioactive isotopes 44Ti and 56Ni are important products of explosive nucleosynthesis, which play a key role in supernova (SN) diagnostics and have been detected in several nearby young SN remnants. However, most SN models based on nonrotating single stars predict yields of 44Ti that are much lower than the va…

2023 The Astrophysical Journal
INTEGRAL 19
Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10-4 Planets from the First 4 yr Survey
DOI: 10.3847/1538-3881/acb34b Bibcode: 2023AJ....165..103Z

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +39 more

We present the analysis of seven microlensing planetary events with planet/host mass ratios q < 10-4: KMT-2017-BLG-1194, KMT-2017-BLG-0428, KMT-2019-BLG-1806, KMT-2017-BLG-1003, KMT-2019-BLG-1367, OGLE-2017-BLG-1806, and KMT-2016-BLG-1105. They were identified by applying the Korea Microlensing Telescope Network (KMTNet) AnomalyFinde…

2023 The Astronomical Journal
eHST 19
The Relationship between Age, Metallicity, and Abundances for Disk Stars in a Simulated Milky Way
DOI: 10.3847/1538-4357/aca1c7 Bibcode: 2023ApJ...942...35C

Ness, Melissa K.; Hawkins, Keith; Wetzel, Andrew +4 more

Observations of the Milky Way's low-α disk show that several element abundances correlate with age at fixed metallicity, with unique slopes and small scatters around the age-[X/Fe] relations. In this study, we turn to simulations to explore the age-[X/Fe] relations for the elements C, N, O, Mg, Si, S, and Ca that are traced in a FIRE-2 cosmologica…

2023 The Astrophysical Journal
Gaia 19
An evolutionary continuum from nucleated dwarf galaxies to star clusters
DOI: 10.1038/s41586-023-06650-z Bibcode: 2023Natur.623..296W

Zhang, Hongxin; Liu, Chengze; Cuillandre, Jean-Charles +21 more

Systematic studies1-4 have revealed hundreds of ultra-compact dwarf galaxies (UCDs5) in the nearby Universe. With half-light radii rh of approximately 10-100 parsecs and stellar masses M* ≈ 106-108 solar masses, UCDs are among the densest known stellar systems6. Although …

2023 Nature
eHST 19
oMEGACat. I. MUSE Spectroscopy of 300,000 Stars within the Half-light Radius of ω Centauri
DOI: 10.3847/1538-4357/acf5db Bibcode: 2023ApJ...958....8N

Dreizler, S.; Milone, A. P.; Latour, M. +17 more

Omega Centauri (ω Cen) is the most massive globular cluster of the Milky Way and has been the focus of many studies that reveal the complexity of its stellar populations and kinematics. However, most previous studies have used photometric and spectroscopic data sets with limited spatial or magnitude coverage, while we aim to investigate it having …

2023 The Astrophysical Journal
Gaia eHST 19
Substructures in Compact Disks of the Taurus Star-forming Region
DOI: 10.3847/1538-4357/acd334 Bibcode: 2023ApJ...952..108Z

Zhang, Ke; Bergin, Edwin A.; Long, Feng +5 more

Observations of substructure in protoplanetary disks have largely been limited to the brightest and largest disks, excluding the abundant population of compact disks, which are likely sites of planet formation. Here, we reanalyze ~0.″1, 1.33 mm Atacama Large Millimeter/submillimeter Array (ALMA) continuum observations of 12 compact protoplanetary …

2023 The Astrophysical Journal
Gaia 19