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JWST study of the DG Tau B disk-wind candidate. I. Overview and nested H2-CO outflows
DOI: 10.1051/0004-6361/202449176 Bibcode: 2024A&A...688A.173D

Podio, L.; Dougados, C.; Tabone, B. +5 more

Context. The origin of outflows and their impact on protoplanetary disk evolution and planet-formation processes are still crucial open questions. DG Tau B is a Class I protostar associated with a structured disk and a rotating conical CO outflow and was recently identified by ALMA as one of the best CO disk wind candidate. It is therefore a perfe…

2024 Astronomy and Astrophysics
JWST 14
Constraints on the narrow-line region of the X-ray quasi-periodic eruption source GSN 069
DOI: 10.1093/mnras/stae1146 Bibcode: 2024MNRAS.530.5120P

Filippenko, Alexei V.; Chiaberge, Marco; Miniutti, Giovanni +5 more

The origins of quasi-periodic eruptions (QPEs) are poorly understood, although most theoretical explanations invoke an accretion disc around a supermassive black hole. The gas and stellar environments in the galactic nuclei of these sources are also poorly constrained. In this paper, we present an analysis of archival Hubble Space Telescope (HST) …

2024 Monthly Notices of the Royal Astronomical Society
eHST 14
O Corona, where art thou? eROSITA's view of UV-optical-IR variability-selected massive black holes in low-mass galaxies
DOI: 10.1051/0004-6361/202347531 Bibcode: 2024A&A...681A..97A

Haberl, F.; Zezas, A.; Georgakakis, A. +16 more

Finding massive black holes (MBHs, MBH ≈ 104-107 M) in the nuclei of low-mass galaxies ≤ft( {{M_*}\mathop {\mathop < \limits_ }\limits_ {{10}10}{M_ ȯ }} \right) is crucial to constrain seeding and growth of black holes over cosmic time, but it is particularly challenging due to their low a…

2024 Astronomy and Astrophysics
XMM-Newton 14
JWST-MIRI Spectroscopy of Warm Molecular Emission and Variability in the AS 209 Disk
DOI: 10.3847/1538-4357/ad20e9 Bibcode: 2024ApJ...964...36R

Banzatti, Andrea; Wilner, David J.; Cleeves, L. Ilsedore +24 more

We present MIRI Medium-resolution Spectrograph observations of the large, multi-gapped protoplanetary disk around the T Tauri star AS 209. The observations reveal hundreds of water vapor lines from 4.9–25.5 µm toward the inner ∼1 au in the disk, including the first detection of rovibrational water emission in this disk. The spectrum is domin…

2024 The Astrophysical Journal
JWST 14
Stellar Cruise Control: Weakened Magnetic Braking Leads to Sustained Rapid Rotation of Old Stars
DOI: 10.3847/1538-4357/ad1516 Bibcode: 2024ApJ...962..138S

Davies, Guy R.; Metcalfe, Travis S.; van Saders, Jennifer L. +8 more

Despite a growing sample of precisely measured stellar rotation periods and ages, the strength of magnetic braking and the degree of departure from standard (Skumanich-like) spin-down have remained persistent questions, particularly for stars more evolved than the Sun. Rotation periods can be measured for stars older than the Sun by leveraging ast…

2024 The Astrophysical Journal
Gaia 14
Extending the chemical reach of the H3 survey: detailed abundances of the dwarf-galaxy stellar stream Wukong/LMS-1
DOI: 10.1093/mnras/stae969 Bibcode: 2024MNRAS.530.2512L

Conroy, Charlie; Ting, Yuan-Sen; Naidu, Rohan P. +10 more

We present the first detailed chemical-abundance analysis of stars from the dwarf-galaxy stellar stream Wukong/LMS-1 covering a wide metallicity range ($-3.5 \lt \rm [Fe/H] \lesssim -1.3$). We find abundance patterns that are effectively indistinguishable from the bulk of Indus and Jhelum, a pair of smaller stellar streams proposed to be dynamical…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 14
The Width of Magnetic Ejecta Measured near 1 au: Lessons from STEREO-A Measurements in 2021–2022
DOI: 10.3847/1538-4357/ad17b9 Bibcode: 2024ApJ...962..193L

Lugaz, Noé; Zhuang, Bin; Scolini, Camilla +7 more

Coronal mass ejections (CMEs) are large-scale eruptions with a typical radial size at 1 au of 0.21 au but their angular width in interplanetary space is still mostly unknown, especially for the magnetic ejecta (ME) part of the CME. We take advantage of STEREO-A angular separation of 20°–60° from the Sun–Earth line from 2020 October to 2022 August,…

2024 The Astrophysical Journal
SOHO 14
A Volume-limited Sample of Ultracool Dwarfs. II. The Substellar Age and Mass Functions in the Solar Neighborhood
DOI: 10.3847/1538-4357/ad39ef Bibcode: 2024ApJ...967..115B

Magnier, Eugene A.; Dupuy, Trent J.; Liu, Michael C. +2 more

We present the most precise constraints to date for the mass and age distributions of single ultracool dwarfs in the solar neighborhood, based on an updated volume-limited sample of 504 L, T, and Y dwarfs within 25 pc. We develop a Monte Carlo approach using the $\langle V/{V}_{\max }\rangle $ statistic to correct for incompleteness and obtain a s…

2024 The Astrophysical Journal
Gaia 14
K2 results for "young" α-rich stars in the Galaxy
DOI: 10.1051/0004-6361/202347440 Bibcode: 2024A&A...683A.111G

Valentini, M.; Chiappini, C.; Tailo, M. +11 more

Context. The origin of apparently young α-rich stars in the Galaxy is still a matter of debate in Galactic archaeology, whether they are genuinely young or might be products of binary evolution, and mergers or mass accretion.
Aims: Our aim is to shed light on the nature of young α-rich stars in the Milky Way by studying their distribution in …

2024 Astronomy and Astrophysics
Gaia 14
MINDS: The DR Tau disk: II. Probing the hot and cold H2O reservoirs in the JWST-MIRI spectrum
DOI: 10.1051/0004-6361/202450355 Bibcode: 2024A&A...689A.330T

Henning, Thomas; Güdel, Manuel; Tabone, Benoît +14 more

Context. The Medium Resolution Spectrometer (MRS) of the Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) gives insights into the chemical richness and complexity of the inner regions of planet-forming disks. Several disks that are compact in the millimetre dust emission have been found by Spitzer to be particularly bright i…

2024 Astronomy and Astrophysics
JWST 14