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The Power of the Rings: The GRB 221009A Soft X-Ray Emission from Its Dust-scattering Halo
DOI: 10.3847/2041-8213/acc1dc Bibcode: 2023ApJ...946L..30T

Pintore, Fabio; Mereghetti, Sandro; Esposito, Paolo +11 more

GRB 221009A is the brightest gamma-ray burst (GRB) ever detected that has occurred at low Galactic latitude. Owing to this exceptional combination, its prompt X-ray emission could be detected for weeks in the form of expanding X-ray rings produced by scattering in Galactic dust clouds. We report on the analysis of 20 rings, generated by dust at di…

2023 The Astrophysical Journal
XMM-Newton 17
Water-rich Disks around Late M Stars Unveiled: Exploring the Remarkable Case of Sz 114
DOI: 10.3847/2041-8213/ad0ed9 Bibcode: 2023ApJ...959L..25X

Zhang, Ke; Pascucci, Ilaria; Banzatti, Andrea +18 more

We present an analysis of the JDISCS JWST/MIRI-MRS spectrum of Sz 114, an accreting M5 star surrounded by a large dust disk with a shallow gap at ~39 au. The spectrum is molecule-rich; we report the detection of water, CO, CO2, HCN, C2H2, and H2. The only identified atomic/ionic transition is from [Ne II…

2023 The Astrophysical Journal
Gaia JWST 17
High-energy Neutrinos from the Inner Circumnuclear Region of NGC 1068
DOI: 10.3847/1538-4357/acee70 Bibcode: 2023ApJ...956....8F

Gallagher, John S.; Lopez Rodriguez, Enrique; Halzen, Francis +1 more

High-energy neutrinos are detected by the IceCube Observatory in the direction of NGC 1068, the archetypical type II Seyfert galaxy. The neutrino flux, surprisingly, is more than an order of magnitude higher than the γ-ray upper limits at measured TeV energy, posing tight constraints on the physical conditions of a neutrino production site. We rep…

2023 The Astrophysical Journal
eHST 17
Rest-frame Near-infrared Radial Light Profiles up to z = 3 from JWST/NIRCam: Wavelength Dependence of the Sérsic Index
DOI: 10.3847/1538-4357/acf716 Bibcode: 2023ApJ...957...46M

Bell, Eric F.; Franx, Marijn; van der Wel, Arjen +10 more

We examine the wavelength dependence of radial light profiles based on Sérsic index n measurements of 1067 galaxies with M * ≥ 109.5 M and in the redshift range 0.5 < z < 3. The sample and rest-frame optical light profiles are drawn from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CA…

2023 The Astrophysical Journal
eHST JWST 17
Fraction of Clumpy Star-forming Galaxies at 0.5 ≤ z ≤ 3 in UVCANDELS: Dependence on Stellar Mass and Environment
DOI: 10.3847/1538-4357/acd5d6 Bibcode: 2023ApJ...951..147S

Grogin, Norman A.; Hathi, Nimish P.; Koekemoer, Anton M. +25 more

High-resolution imaging of galaxies in rest-frame UV has revealed the existence of giant star-forming clumps prevalent in high-redshift galaxies. Studying these substructures provides important information about their formation and evolution and informs theoretical galaxy evolution models. We present a new method to identify clumps in galaxies' hi…

2023 The Astrophysical Journal
eHST 17
Early Results from GLASS-JWST. XXIII. The Transmission of Lyα from UV-faint z 3-6 Galaxies
DOI: 10.3847/1538-4357/acf715 Bibcode: 2023ApJ...956..136P

Castellano, Marco; Pentericci, Laura; Treu, Tommaso +18 more

Lyα emission from galaxies can be used to trace neutral hydrogen in the epoch of reionization, however, there is a degeneracy between the attenuation of Lyα in the intergalactic medium (IGM) and the line profile emitted by the galaxy. Large shifts of Lyα redward of systemic due to scattering in the interstellar medium can boost Lyα transmission in…

2023 The Astrophysical Journal
eHST JWST 17
Precise Empirical Determination of Metallicity Dependence of Near-infrared Period-Luminosity Relations for RR Lyrae Variables
DOI: 10.3847/2041-8213/acba7f Bibcode: 2023ApJ...944L..51B

de Grijs, Richard; Marconi, Marcella; Dall'Ora, Massimo +9 more

RR Lyrae variables are excellent Population II distance indicators thanks to their well-defined period-luminosity relations (PLRs) at infrared wavelengths. We present results of near-infrared (NIR) monitoring of Galactic globular clusters to empirically quantify the metallicity dependence of NIR PLRs for RR Lyrae variables. Our sample includes hom…

2023 The Astrophysical Journal
Gaia 17
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XXIV. Differences in Internal Kinematics of Multiple Stellar Populations
DOI: 10.3847/1538-4357/acaec6 Bibcode: 2023ApJ...944...58L

Brown, Thomas M.; Milone, Antonino P.; Vesperini, Enrico +12 more

Our understanding of the kinematic properties of multiple stellar populations (mPOPs) in Galactic globular clusters (GCs) is still limited compared to what we know about their chemical and photometric characteristics. Such limitation arises from the lack of a comprehensive observational investigation of this topic. Here we present the first homoge…

2023 The Astrophysical Journal
eHST 17
A Type II Radio Burst Driven by a Blowout Jet on the Sun
DOI: 10.3847/1538-4357/ace31b Bibcode: 2023ApJ...953..171H

Tian, Hui; Madjarska, Maria S.; Deng, Yuanyong +5 more

Type II radio bursts are often associated with coronal shocks that are typically driven by coronal mass ejections (CMEs) from the Sun. Here we conduct a case study of a type II radio burst that is associated with a C4.5-class flare and a blowout jet, but without the presence of a CME. The blowout jet is observed near the solar disk center in the e…

2023 The Astrophysical Journal
SOHO 17
Carbon Stars as Standard Candles: An Empirical Test for the Reddening, Metallicity, and Age Sensitivity of the J-region Asymptotic Giant Branch (JAGB) Method
DOI: 10.3847/1538-4357/acee69 Bibcode: 2023ApJ...956...15L

Lee, Abigail J.

The J-region Asymptotic Giant Branch (JAGB) method is a standard candle based on the intrinsic luminosities of carbon stars in the near-infrared. We directly constrain the impact of metallicity, age, and reddening on the JAGB method. We assess how the mode, skew, and spread of the JAGB star LF change throughout diverse stellar environments in M31'…

2023 The Astrophysical Journal
eHST 16