Search Publications

Robust Evidence for the Breakdown of Standard Gravity at Low Acceleration from Statistically Pure Binaries Free of Hidden Companions
DOI: 10.3847/1538-4357/ad0ed5 Bibcode: 2024ApJ...960..114C

Chae, Kyu-Hyun

It is found that Gaia Data Release 3 binary stars selected with stringent requirements on astrometric measurements and radial velocities naturally satisfy Newtonian dynamics without hidden close companions when the projected separation s ≲ 2 kau, showing that pure binaries can be selected. It is then found that pure binaries selected with the same…

2024 The Astrophysical Journal
Gaia 31
Gaia's binary star renaissance
DOI: 10.1016/j.newar.2024.101694 Bibcode: 2024NewAR..9801694E

El-Badry, Kareem

Stellar multiplicity is among the oldest and richest problems in astrophysics. Binary stars are a cornerstone of stellar mass and radius measurements that underpin modern stellar evolutionary models. Binaries are the progenitors of many of the most interesting and exotic astrophysical phenomena, ranging from type Ia supernovae to gamma ray bursts,…

2024 New Astronomy Reviews
Gaia 31
Outshining in the spatially resolved analysis of a strongly lensed galaxy at z = 6.072 with JWST NIRCam
DOI: 10.1051/0004-6361/202349135 Bibcode: 2024A&A...686A..63G

Magdis, G. E.; Laporte, N.; Mason, C. A. +19 more

We present JWST/NIRCam observations of a strongly lensed, sub-L*, multiply imaged galaxy at z = 6.072, with magnification factors µ ≳ 20 across the galaxy. The galaxy has rich HST, MUSE, and ALMA ancillary observations across a broad wavelength range. Aiming to quantify the reliability of stellar mass estimates of high redshift ga…

2024 Astronomy and Astrophysics
JWST 31
Discovery of a variable energy-dependent X-ray polarization in the accreting neutron star GX 5−1
DOI: 10.1051/0004-6361/202347374 Bibcode: 2024A&A...684A.137F

Kaaret, Philip; Wu, Kinwah; Steiner, James F. +116 more

We report on the coordinated observations of the neutron star low-mass X-ray binary (NS-LMXB) GX 5−1 in X-rays (IXPE, NICER, NuSTAR, and INTEGRAL), optical (REM and LCO), near-infrared (REM), mid-infrared (VLT VISIR), and radio (ATCA). This Z-source was observed by IXPE twice in March-April 2023 (Obs. 1 and 2). In the radio band the source was det…

2024 Astronomy and Astrophysics
INTEGRAL 31
UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at z spec = 3.97
DOI: 10.3847/1538-4357/ad6a18 Bibcode: 2024ApJ...974..145S

Glazebrook, Karl; Nanayakkara, Themiya; van Dokkum, Pieter +28 more

We report the spectroscopic confirmation of a massive ( log(M/M

2024 The Astrophysical Journal
JWST 31
Ionized Gas Kinematics with FRESCO: An Extended, Massive, Rapidly Rotating Galaxy at z = 5.4
DOI: 10.3847/2041-8213/ad7b17 Bibcode: 2024ApJ...976L..27N

Maseda, Michael V.; Übler, Hannah; Bunker, Andrew J. +43 more

With the remarkable sensitivity and resolution of JWST in the infrared, measuring rest-optical kinematics of galaxies at z > 5 has become possible for the first time. This study pilots a new method for measuring galaxy dynamics for highly multiplexed, unbiased samples by combining FRESCO NIRCam grism spectroscopy and JADES medium-band imaging. …

2024 The Astrophysical Journal
JWST 31
Diverse Oxygen Abundance in Early Galaxies Unveiled by Auroral Line Analysis with JWST
DOI: 10.3847/1538-4357/ad5290 Bibcode: 2024ApJ...971...43M

Stiavelli, Massimo; Treu, Tommaso; Trenti, Michele +10 more

We present deep JWST NIRSpec observations in the sight line of MACS J1149.5+2223, a massive cluster of galaxies at z = 0.54. We report the spectroscopic redshift of 28 sources at 3 < z < 9.1, including nine sources with the detection of the

2024 The Astrophysical Journal
eHST JWST 31
Stellar flares
DOI: 10.1007/s41116-024-00039-4 Bibcode: 2024LRSP...21....1K

Kowalski, Adam F.

Magnetic storms on stars manifest as remarkable, randomly occurring changes of the luminosity over durations that are tiny in comparison to the normal evolution of stars. These stellar flares are bursts of electromagnetic radiation from X-ray to radio wavelengths, and they occur on most stars with outer convection zones. They are analogous to the …

2024 Living Reviews in Solar Physics
Gaia 31
Testing EMRI Models for Quasi-periodic Eruptions with 3.5 yr of Monitoring eRO-QPE1
DOI: 10.3847/1538-4357/ad2941 Bibcode: 2024ApJ...965...12C

Remillard, Ronald A.; Maccarone, Thomas J.; Burdge, Kevin B. +13 more

Quasi-periodic eruptions (QPEs) are luminous X-ray outbursts recurring on hour timescales, observed from the nuclei of a growing handful of nearby low-mass galaxies. Their physical origin is still debated, and usually modeled as (a) accretion disk instabilities or (b) interaction of a supermassive black hole (SMBH) with a lower mass companion in a…

2024 The Astrophysical Journal
XMM-Newton 30
Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13
DOI: 10.3847/1538-4357/ad7d03 Bibcode: 2024ApJ...975..178K

Finkelstein, Steven L.; Casey, Caitlin M.; Larson, Rebecca L. +8 more

The James Webb Space Telescope (JWST) has uncovered a ubiquitous population of dust-obscured compact sources at z ≳ 4. Many of these objects exhibit signs of active galactic nucleus (AGN) activity, making their study crucial for understanding the formation of supermassive black holes (SMBHs) and their growth with host galaxies. In this work, we ex…

2024 The Astrophysical Journal
JWST 30