Search Publications

The Ages of Galactic Bulge Stars with Realistic Uncertainties
DOI: 10.3847/1538-4357/acb692 Bibcode: 2023ApJ...946...28J

Rich, R. Michael; Johnson, Christian I.; Joyce, Meridith +3 more

Using modern isochrones with customized physics and carefully considered statistical techniques, we recompute the age distribution for a sample of 91 microlensed dwarfs in the Galactic bulge presented by Bensby et al. and do not produce an age distribution consistent with their results. In particular, our analysis finds that only 15 of 91 stars ha…

2023 The Astrophysical Journal
Gaia eHST 37
A real-time transient detector and the living Swift-XRT point source catalogue
DOI: 10.1093/mnras/stac2937 Bibcode: 2023MNRAS.518..174E

Cenko, S. B.; Campana, S.; Kennea, J. A. +5 more

We present the Living Swift-XRT Point Source (LSXPS) catalogue and real-time transient detector. This system allows us for the first time to carry out low-latency searches for new transient X-ray events fainter than those available to the current generation of wide-field imagers, and report their detection in near real time. Previously, such event…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 37
A calibration point for stellar evolution from massive star asteroseismology
DOI: 10.1038/s41550-023-01978-y Bibcode: 2023NatAs...7..913B

Bowman, Dominic M.; Vanderspek, Roland; Aerts, Conny +10 more

Massive stars are progenitors of supernovae, neutron stars and black holes. During the hydrogen-core burning phase, their convective cores are the prime drivers of their evolution, but inferences of core masses are subject to unconstrained boundary mixing processes. Moreover, uncalibrated transport mechanisms can lead to strong envelope mixing and…

2023 Nature Astronomy
Gaia 37
The diverse chemistry of protoplanetary disks as revealed by JWST
DOI: 10.1039/D3FD00010A Bibcode: 2023FaDi..245...52V

Kamp, I.; Henning, Th.; Nazari, P. +14 more

Early results from JWST-MIRI programs on low- and high-mass protostars and disks show significant diversity in their mid-infrared spectra, most notably for CO2, H2O and C2H2. Benzene is detected in disks around very low mass stars. Early results from the James Webb Space Telescope-Mid-InfraRed Instrument (JWST-MIRI) guaranteed time programs on pro…

2023 Faraday Discussions
Gaia 36
Potential Atmospheric Compositions of TRAPPIST-1 c Constrained by JWST/MIRI Observations at 15 µm
DOI: 10.3847/2041-8213/acee02 Bibcode: 2023ApJ...955L...7L

Kreidberg, Laura; Meadows, Victoria S.; Lincowski, Andrew P. +13 more

The first James Webb Space Telescope observations of TRAPPIST-1 c showed a secondary eclipse depth of 421 ± 94 ppm at 15 µm, which is consistent with a bare rock surface or a thin, O2-dominated, low-CO2 atmosphere. Here we further explore potential atmospheres for TRAPPIST-1 c by comparing the observed secondary eclipse…

2023 The Astrophysical Journal
JWST 36
TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf
DOI: 10.3847/1538-3881/acabce Bibcode: 2023AJ....165..120K

Kobulnicky, Henry A.; Cochran, William D.; Mahadevan, Suvrath +27 more

We present the discovery of TOI-5205b, a transiting Jovian planet orbiting a solar metallicity M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometry and then confirmed using a combination of precise radial velocities, ground-based photometry, spectra, and speckle imaging. TOI-5205b has one of the highest mass ratios…

2023 The Astronomical Journal
Gaia 36
Detailed Chemical Abundances of Stars in the Outskirts of the Tucana II Ultrafaint Dwarf Galaxy
DOI: 10.3847/1538-3881/aca416 Bibcode: 2023AJ....165...55C

Jerjen, Helmut; Frebel, Anna; Simon, Joshua D. +6 more

We present chemical abundances and velocities of five stars between 0.3 and 1.1 kpc from the center of the Tucana II ultrafaint dwarf galaxy (UFD) from high-resolution Magellan/MIKE spectroscopy. We find that every star is deficient in metals (-3.6 < [Fe/H] < -1.9) and in neutron-capture elements as is characteristic of UFD stars, unambiguou…

2023 The Astronomical Journal
Gaia 36
HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
DOI: 10.1007/s11214-023-01019-0 Bibcode: 2023SSRv..219...74K

Verscharen, Daniel; Retinò, Alessandro; Alexandrova, Olga +47 more

HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in plasmas throughout the universe. This will be accomplished by making simultaneous measurements at ni…

2023 Space Science Reviews
Cluster 36
PHANGS-JWST First Results: Mapping the 3.3 µm Polycyclic Aromatic Hydrocarbon Vibrational Band in Nearby Galaxies with NIRCam Medium Bands
DOI: 10.3847/2041-8213/acb0cf Bibcode: 2023ApJ...944L...7S

Sandstrom, Karin M.; Bolatto, Alberto D.; Kruijssen, J. M. Diederik +28 more

We present maps of the 3.3 µm polycyclic aromatic hydrocarbon (PAH) emission feature in NGC 628, NGC 1365, and NGC 7496 as observed with the Near-Infrared Camera imager on JWST from the PHANGS-JWST Cycle 1 Treasury project. We create maps that isolate the 3.3 µm PAH feature in the F335M filter (F335MPAH) using combinations o…

2023 The Astrophysical Journal
JWST 36
Photometric binaries, mass functions, and structural parameters of 78 Galactic open clusters
DOI: 10.1051/0004-6361/202245457 Bibcode: 2023A&A...672A..29C

Milone, Antonino P.; Vesperini, Enrico; Lagioia, Edoardo P. +8 more

Context. Binary stars play a crucial role in our understanding of the formation and evolution of star clusters and their stellar populations.
Aims: We use Gaia Data Release 3 to homogeneously analyze 78 Galactic open clusters and the unresolved binary systems they host, each composed of two main sequence (MS) stars.
Methods: We first inv…

2023 Astronomy and Astrophysics
Gaia 36