Search Publications

Constraints on the dense matter equation of state from young and cold isolated neutron stars
DOI: 10.1038/s41550-024-02291-y Bibcode: 2024NatAs...8.1020M

Rea, N.; Marino, A.; Pons, J. A. +3 more

Neutron stars are the dense and highly magnetic relics of supernova explosions of massive stars. The quest to constrain the equation of state (EOS) of ultradense matter and thereby probe the behaviour of matter inside neutron stars is one of the core goals of modern physics and astrophysics. A promising method involves investigating the long-term …

2024 Nature Astronomy
XMM-Newton 10
Dark energy survey year 3 results: miscentring calibration and X-ray-richness scaling relations in redMaPPer clusters
DOI: 10.1093/mnras/stae1786 Bibcode: 2024MNRAS.533..572K

Bacon, D.; Smith, M.; Davis, T. M. +77 more

We use Dark Energy Survey Year 3 (DES Y3) clusters with archival XMM-Newton and Chandra X-ray data to assess the centring performance of the redMaPPer cluster finder and to measure key richness observable scaling relations. We find that 10-20 per cent of redMaPPer clusters are miscentred, both when comparing to the X-ray peak position and to the v…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 10
Modeling and Subtracting Diffuse Cluster Light in JWST Images: A Relation between the Spatial Distribution of Globular Clusters, Dwarf Galaxies, and Intracluster Light in the Lensing Cluster SMACS 0723
DOI: 10.3847/1538-4357/ad7735 Bibcode: 2024ApJ...975...76M

Willott, Chris J.; Harshan, Anishya; Martis, Nicholas S. +11 more

We present a methodology for modeling and removing light from cluster galaxies and intracluster light (ICL) from James Webb Space Telescope images of gravitational lensing clusters. We apply our method to Webb's First Deep Field the SMACS 0723 Early Release Observations and use the ICL-subtracted images to select a sample of globular clusters (GCs…

2024 The Astrophysical Journal
eHST JWST 10
Chemical tracers of a highly eccentric AGB-main-sequence star binary
DOI: 10.1038/s41550-023-02154-y Bibcode: 2024NatAs...8..308D

Menten, K. M.; Pinte, C.; Sahai, R. +32 more

Binary interactions have been proposed to explain a variety of circumstellar structures seen around evolved stars, including asymptotic giant branch (AGB) stars and planetary nebulae. Studies resolving the circumstellar envelopes of AGB stars have revealed spirals, disks and bipolar outflows, with shaping attributed to interactions with a companio…

2024 Nature Astronomy
eHST 10
Detection of the elusive dangling OH ice features at ~2.7 µm in Chamaeleon I with JWST NIRCam
DOI: 10.1038/s41550-024-02307-7 Bibcode: 2024NatAs...8.1169N

Sun, F.; Egami, E.; Rocha, W. R. M. +31 more

Ascertaining the morphology and composition of the icy mantles covering dust grains in dense, cold regions of the interstellar medium is essential to developing accurate astrochemical models, determining conditions for ice formation, constraining chemical interactions in and on icy grains and understanding how ices withstand space radiation. The w…

2024 Nature Astronomy
JWST 10
Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-time Distribution
DOI: 10.3847/1538-4357/ad61df Bibcode: 2024ApJ...973...55D

Johnson, Jennifer A.; Johnson, James W.; Dubay, Liam O.

Type Ia supernovae (SNe Ia) produce most of the Fe-peak elements in the Universe and therefore are a crucial ingredient in galactic chemical evolution models. SNe Ia do not explode immediately after star formation, and the delay-time distribution (DTD) has not been definitively determined by supernova surveys or theoretical models. Because the DTD…

2024 The Astrophysical Journal
Gaia 10
Unveiling δ Scuti and γ Doradus hybrid pulsation of HD 53166 and HD 53349 plus rich frequencies in HD 52788
DOI: 10.1016/j.newast.2023.102081 Bibcode: 2024NewA..10502081Z

Zhou, Ai-Ying

We present discoveries of the hybrid δ Scuti and γ Doradus types stellar pulsational variability of two stars, HD 53166 and HD 53349, which were previously used as comparison in the differential photometry of a known δ Scuti star HD 52788. More surprisingly, HD 52788 exhibits 126 pulsation frequencies in a small domain in 4-12 d-1 based…

2024 New Astronomy
Gaia 10
ReveaLLAGN 0: First Look at JWST MIRI Data of Sombrero and NGC 1052
DOI: 10.3847/1538-4357/ad3065 Bibcode: 2024ApJ...966..204G

Kirkpatrick, Allison; Trump, Jonathan R.; Lützgendorf, Nora +28 more

We present the first results from the Revealing Low-Luminosity Active Galactic Nuclei (ReveaLLAGN) survey, a JWST survey of seven nearby LLAGNs. We focus on two observations with the Mid-Infrared Instrument (MIRI)'s Medium-Resolution Spectrometer of the nuclei of NGC 1052 and Sombrero (NGC 4594/M104). We also compare these data to public JWST data…

2024 The Astrophysical Journal
Gaia JWST 10
Uniting Gaia and APOGEE to unveil the cosmic chemistry of the Milky Way disc
DOI: 10.1051/0004-6361/202348018 Bibcode: 2024A&A...683A.128C

Casey, Andrew R.; Rix, Hans-Walter; Brown, Anthony G. A. +6 more

The spatial distribution of Galactic stars with different chemical abundances encodes information on the processes that drove the formation and evolution of the Milky Way. Survey selection functions are indispensable for analysing astronomical catalogues produced by large-scale surveys. The use of these selection functions in data modelling is mor…

2024 Astronomy and Astrophysics
Gaia 10
Lyα Emission Line Profiles of Extreme [O III]- emitting Galaxies at z ≳ 2: Implications for Lyα Visibility in the Reionization Era
DOI: 10.3847/1538-4357/ad5ae0 Bibcode: 2024ApJ...972...56T

Tang, Mengtao; Stark, Daniel P.; Ellis, Richard S. +4 more

JWST observations have recently begun delivering the first samples of Lyα velocity profile measurements at z > 6, opening a new window into the reionization process. Interpretation of z ≳ 6 line profiles is currently stunted by limitations in our knowledge of the intrinsic Lyα profile (before encountering the intergalactic medium (IGM)) of the …

2024 The Astrophysical Journal
eHST JWST 10