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The APO-K2 Catalog. I. 7500 Red Giants with Fundamental Stellar Parameters from APOGEE DR17 Spectroscopy and K2-GAP Asteroseismology
DOI: 10.3847/1538-3881/ad0b13 Bibcode: 2024AJ....167...50S

Pinsonneault, Marc; Stassun, Keivan G.; García, Rafael A. +14 more

We present a catalog of fundamental stellar properties for ~7500 evolved stars, including stellar radii and masses, determined from the combination of spectroscopic observations from the Apache Point Observatory Galactic Evolution Experiment, part of the Sloan Digital Sky Survey IV, and asteroseismology from K2. The resulting APO-K2 catalog provid…

2024 The Astronomical Journal
Gaia 22
RR Lyrae from binary evolution: abundant, young, and metal-rich
DOI: 10.1093/mnras/stad3996 Bibcode: 2024MNRAS.52712196B

Belokurov, Vasily; Bobrick, Alexey; Iorio, Giuliano +3 more

RR Lyrae are a well-known class of pulsating horizontal branch stars widely used as tracers of old, metal-poor stellar populations. However, mounting observational evidence shows that a significant fraction of these stars may be young and metal-rich. Here, through detailed binary stellar evolution modelling, we show that all such metal-rich RR Lyr…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 22
Transmission Spectroscopy of the Habitable Zone Exoplanet LHS 1140 b with JWST/NIRISS
DOI: 10.3847/2041-8213/ad5afa Bibcode: 2024ApJ...970L...2C

MacDonald, Ryan J.; Dang, Lisa; Cowan, Nicolas B. +20 more

LHS 1140 b is the second-closest temperate transiting planet to Earth with an equilibrium temperature low enough to support surface liquid water. At 1.730 ± 0.025 R , LHS 1140 b falls within the radius valley separating H2-rich mini-Neptunes from rocky super-Earths. Recent mass and radius revisions indicate a bulk density si…

2024 The Astrophysical Journal
Gaia JWST 22
Gaia DR3 data consistent with a short bar connected to a spiral arm
DOI: 10.1093/mnras/stae083 Bibcode: 2024MNRAS.528.3576V

Steinmetz, M.; Khoperskov, S.; Minchev, I. +8 more

We use numerical simulations to model Gaia DR3 data with the aim of constraining the Milky Way (MW) bar and spiral structure parameters. We show that both the morphology and the velocity field in MW-like galactic disc models are strong functions of time, changing dramatically over a few tens of Myr. This suggests that by finding a good match to th…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 22
Evidence for inflows and outflows in the nearby black hole transient Swift J1727.8−162
DOI: 10.1051/0004-6361/202348754 Bibcode: 2024A&A...682L...1M

Armas Padilla, M.; Mata Sánchez, D.; Muñoz-Darias, T. +2 more

We present 20 epochs of optical spectroscopy obtained with the GTC-10.4m telescope across the bright discovery outburst of the black hole candidate Swift J1727.8−162. The spectra cover the main accretion states and are characterised by the presence of hydrogen and helium emission lines, commonly observed in these objects. They show complex profile…

2024 Astronomy and Astrophysics
Gaia 22
THEMIS 2.0: A self-consistent model for dust extinction, emission, and polarisation
DOI: 10.1051/0004-6361/202348391 Bibcode: 2024A&A...684A..34Y

Miville-Deschênes, M. -A.; Ysard, N.; Guillet, V. +6 more

Context. Recent observational constraints in emission, extinction, and polarisation have at least partially invalidated most of the astronomical standard grain models for the diffuse interstellar medium. Moreover, laboratory measurements on interstellar silicate analogues have shown quite significant differences with the optical properties used in…

2024 Astronomy and Astrophysics
Herschel 21
The ALMA-CRISTAL survey: Widespread dust-obscured star formation in typical star-forming galaxies at z = 4–6
DOI: 10.1051/0004-6361/202348782 Bibcode: 2024A&A...690A.197M

Übler, Hannah; Ferrara, Andrea; Fisher, Deanne B. +29 more

We present the morphological parameters and global properties of dust-obscured star formation in typical star-forming galaxies at z = 4–6. Among 26 galaxies composed of 20 galaxies observed by the Cycle-8 ALMA Large Program, CRISTAL, and 6 galaxies from archival data, we individually detect rest-frame 158 µm dust continuum emission from 19 g…

2024 Astronomy and Astrophysics
eHST 21
Sulfur Dioxide and Other Molecular Species in the Atmosphere of the Sub-Neptune GJ 3470 b
DOI: 10.3847/2041-8213/ad55e9 Bibcode: 2024ApJ...970L..10B

Fortney, Jonathan J.; Henry, Gregory W.; Bell, Taylor J. +13 more

We report observations of the atmospheric transmission spectrum of the sub-Neptune exoplanet GJ 3470 b taken using the Near-Infrared Camera on JWST. Combined with two archival Hubble Space Telescope/Wide-Field Camera 3 transit observations and 15 archival Spitzer transit observations, we detect water, methane, sulfur dioxide, and carbon dioxide in…

2024 The Astrophysical Journal
Gaia eHST JWST 21
A Walk on the Retrograde Side (WRS) project. I. Tidying-up the retrograde halo with high-resolution spectroscopy
DOI: 10.1051/0004-6361/202348332 Bibcode: 2024A&A...684A..37C

Ilyin, I.; Lardo, C.; Massari, D. +7 more

Relics of ancient accretion events experienced by the Milky Way are predominantly located within the stellar halo of our Galaxy. However, debris from different objects display overlapping distributions in dynamical spaces, making it extremely challenging to properly disentangle their contribution to the build-up of the Galaxy. To shed light on thi…

2024 Astronomy and Astrophysics
Gaia 21
Uncovering a Massive z 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
DOI: 10.3847/2041-8213/ad11ee Bibcode: 2024ApJ...961L..25L

Casey, Caitlin M.; Chworowsky, Katherine; Hutchison, Taylor A. +47 more

In this Letter, we report the discovery of the highest redshift, heavily obscured, radio-loud (RL) active galactic nucleus (AGN) candidate selected using JWST NIRCam/MIRI, mid-IR, submillimeter, and radio imaging in the COSMOS-Web field. Using multifrequency radio observations and mid-IR photometry, we identify a powerful, RL, growing supermassive…

2024 The Astrophysical Journal
eHST JWST 21