Search Publications

Fast-moving stars around an intermediate-mass black hole in ω Centauri
DOI: 10.1038/s41586-024-07511-z Bibcode: 2024Natur.631..285H

Anderson, Jay; Pechetti, Renuka; Kamann, Sebastian +15 more

Black holes have been found over a wide range of masses, from stellar remnants with masses of 5-150 solar masses (M), to those found at the centres of galaxies with M > 105M. However, only a few debated candidate black holes exist between 150M and 105M. Determining the popula…

2024 Nature
Gaia eHST 52
LISA Galactic Binaries with Astrometry from Gaia DR3
DOI: 10.3847/1538-4357/ad2068 Bibcode: 2024ApJ...963..100K

Ramsay, Gavin; Kupfer, Thomas; Pala, Anna F. +11 more

Galactic compact binaries with orbital periods shorter than a few hours emit detectable gravitational waves (GWs) at low frequencies. Their GW signals can be detected with the future Laser Interferometer Space Antenna (LISA). Crucially, they may be useful in the early months of the mission operation in helping to validate LISA's performance in com…

2024 The Astrophysical Journal
Gaia 52
In-situ versus accreted Milky Way globular clusters: a new classification method and implications for cluster formation
DOI: 10.1093/mnras/stad3920 Bibcode: 2024MNRAS.528.3198B

Belokurov, Vasily; Kravtsov, Andrey

We present a new scheme for the classification of the in-situ and accreted globular clusters (GCs). The scheme uses total energy E and z-component of the orbital angular momentum and is calibrated using the [Al/Fe] abundance ratio. We demonstrate that this classification results in two GC populations with distinct spatial, kinematic, and chemical …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 51
The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S
DOI: 10.3847/1538-4357/ad0da7 Bibcode: 2024ApJ...962..124H

Maiolino, Roberto; Willott, Chris; Johnson, Benjamin D. +28 more

We report the discovery of an extreme galaxy overdensity at z = 5.4 in the GOODS-S field using James Webb Space Telescope (JWST)/NIRCam imaging from JADES and JEMS alongside JWST/NIRCam wide-field slitless spectroscopy from FRESCO. We identified potential members of the overdensity using Hubble Space Telescope+JWST photometry spanning λ = 0.4–5.0 …

2024 The Astrophysical Journal
Gaia eHST JWST 51
The JWST Discovery of the Triply Imaged Type Ia "Supernova H0pe" and Observations of the Galaxy Cluster PLCK G165.7+67.0
DOI: 10.3847/1538-4357/ad1034 Bibcode: 2024ApJ...961..171F

Grogin, Norman A.; Koekemoer, Anton M.; Pirzkal, Nor +38 more

A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35). The SN is situated 1.5–2 kpc from the host-galaxy nucleus and appears in three different locations as a result of gravitational lensing by G165. These data can yield a value for Hub…

2024 The Astrophysical Journal
Gaia eHST JWST 51
A shock flash breaking out of a dusty red supergiant
DOI: 10.1038/s41586-023-06843-6 Bibcode: 2024Natur.627..754L

Wang, Lifan; Wang, Xiaofeng; Gao, Xing +41 more

Shock-breakout emission is light that arises when a shockwave, generated by the core-collapse explosion of a massive star, passes through its outer envelope. Hitherto, the earliest detection of such a signal was at several hours after the explosion1, although a few others had been reported2-7. The temporal evolution of early …

2024 Nature
Gaia 50
Undermassive Host Galaxies of Five z ∼ 6 Luminous Quasars Detected with JWST
DOI: 10.3847/1538-4357/ad2a57 Bibcode: 2024ApJ...964...90S

Lyu, Jianwei; Rieke, George H.; Alberts, Stacey +2 more

We measure host galaxy stellar masses for a sample of five luminous quasars at z ∼ 5–7. Using JWST/NIRCam medium-band images of nearby point-spread function reference stars, we carefully subtract the contribution from the quasar light to place upper and lower limits on the flux of each host galaxy. We find that the members of our sample of quasar …

2024 The Astrophysical Journal
JWST 50
The Small Sizes and High Implied Densities of "Little Red Dots" with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus
DOI: 10.3847/2041-8213/ad90b8 Bibcode: 2024ApJ...977L..13B

Maseda, Michael V.; Franx, Marijn; Labbé, Ivo +10 more

Early JWST studies found an apparent population of massive, compact galaxies at redshifts z ≳ 7. Recently three of these galaxies were shown to have prominent Balmer breaks, demonstrating that their light at λrest ∼ 3500 Å is dominated by a stellar population that is relatively old (∼200 Myr). All three also have broad Hβ emission with …

2024 The Astrophysical Journal
JWST 50
JWST Observations of Young protoStars (JOYS+): Detecting icy complex organic molecules and ions. I. CH4, SO2, HCOO, OCN, H2CO, HCOOH, CH3CH2OH, CH3CHO, CH3OCHO, and CH3COOH
DOI: 10.1051/0004-6361/202348427 Bibcode: 2024A&A...683A.124R

Ray, T. P.; Chen, Y.; Henning, Th. +23 more

Context. Complex organic molecules (COMs) are ubiquitously detected in the gas phase and thought to be mostly formed on icy grains. Nevertheless, there have not been any unambiguous detections of COMs larger than CH3OH in ices reported thus far. Exploring this matter in greater detail has now become possible with the unprecedented possi…

2024 Astronomy and Astrophysics
JWST 50
Deciphering Lyman-α emission deep into the epoch of reionization
DOI: 10.1038/s41550-023-02179-3 Bibcode: 2024NatAs...8..384W

Pérez-González, Pablo G.; Santini, Paola; Grogin, Norman A. +18 more

During the epoch of reionization, the first galaxies were enshrouded in pristine neutral gas, with one of the brightest emission lines in star-forming galaxies, Lyman α (Lyα), expected to remain undetected until the Universe became ionized. Providing an explanation for the surprising detection of Lyα in these early galaxies is a major challenge fo…

2024 Nature Astronomy
eHST JWST 50