Search Publications

Was There a 3.5 keV Line?
DOI: 10.3847/1538-4357/ad2612 Bibcode: 2024ApJ...964..185D

Safdi, Benjamin R.; Foster, Joshua W.; Dessert, Christopher +1 more

The 3.5 keV line is a purported emission line observed in galaxies, galaxy clusters, and the Milky Way whose origin is inconsistent with known atomic transitions and has previously been suggested to arise from dark matter decay. We systematically reexamine the bulk of the evidence for the 3.5 keV line, attempting to reproduce six previous analyses…

2024 The Astrophysical Journal
XMM-Newton 14
A JWST/MIRI and NIRCam Analysis of the Young Stellar Object Population in the Spitzer I Region of NGC 6822
DOI: 10.3847/1538-4357/ad3f90 Bibcode: 2024ApJ...967..110L

Temim, Tea; Hirschauer, Alec S.; Boyer, Martha L. +8 more

We present an imaging survey of the Spitzer I star-forming region in NGC 6822 conducted with the NIRCam and MIRI instruments on board JWST. Located at a distance of 490 kpc, NGC 6822 is the nearest non-interacting low-metallicity (∼0.2 Z ) dwarf galaxy. It hosts some of the brightest known H II regions in the local universe, including …

2024 The Astrophysical Journal
JWST 14
Witnessing an extreme, highly efficient galaxy formation mode with resolved Lyman-α and Lyman-continuum emission
DOI: 10.1051/0004-6361/202451667 Bibcode: 2024A&A...691A..87M

Chisholm, J.; Schaerer, D.; Marques-Chaves, R. +9 more

J1316+2614 at z = 3.613 is the UV-brightest (MUV = ‑24.7) and strongest Lyman continuum-emitting (fescLyC ≈ 90%) star-forming galaxy known; it also shows signatures of inflowing gas from its blue-dominated Lyα profile. We present high-resolution imaging with the Hubble Space Telescope (HST) and the Very Large Teles…

2024 Astronomy and Astrophysics
Gaia eHST 14
Narrow-line Seyfert 1 galaxies in Sloan Digital Sky Survey: a new optical spectroscopic catalogue
DOI: 10.1093/mnras/stad3650 Bibcode: 2024MNRAS.527.7055P

Stalin, C. S.; Saikia, D. J.; Domínguez, Alberto +1 more

Narrow-line Seyfert 1 (NLSy1) galaxies are an enigmatic class of active galactic nuclei (AGN) that exhibit peculiar multiwavelength properties across the electromagnetic spectrum. For example, these sources have allowed us to explore the innermost regions of the central engine of AGN using X-ray observations and have also provided clues about the …

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 14
Galactic 'Snake' IRDC G11.11-0.12: a site of multiple hub-filament systems and colliding filamentary clouds
DOI: 10.1093/mnras/stad3384 Bibcode: 2024MNRAS.527.5895D

Dewangan, L. K.; Sharma, Saurabh; Eswaraiah, C. +3 more

To probe star formation processes, we present a multiscale and multiwavelength investigation of the 'Snake' nebula/infrared dark cloud G11.11-0.12 (hereafter, G11; length ~27 pc). Spitzer images hint at the presence of subfilaments (in absorption), and reveal four infrared-dark hub-filament system (HFS) candidates (extent < 6 pc) towards G11, w…

2024 Monthly Notices of the Royal Astronomical Society
Herschel JWST 14
[X/Fe] Marks the Spot: Mapping Chemical Azimuthal Variations in the Galactic Disk with APOGEE
DOI: 10.3847/1538-4357/ad900e Bibcode: 2024ApJ...977..143H

Laporte, Chervin F. P.; Price-Whelan, Adrian M.; Horta, Danny +4 more

Chemical cartography of the Galactic disk provides insights into its structure and assembly history over cosmic time. In this work, we use chemical cartography to explore chemical gradients and azimuthal substructure in the Milky Way disk with giant stars from Apache Point Observatory Galactic Evolution Experiment (APOGEE) DR17. We confirm the exi…

2024 The Astrophysical Journal
Gaia 14
A Two-Component Probability Distribution Function Describes the Mid-IR Emission from the Disks of Star-forming Galaxies
DOI: 10.3847/1538-3881/ad110d Bibcode: 2024AJ....167...39P

Sandstrom, Karin M.; Ramambason, Lise; Leroy, Adam K. +28 more

High-resolution JWST-MIRI images of nearby spiral galaxies reveal emission with complex substructures that trace dust heated both by massive young stars and the diffuse interstellar radiation field. We present high angular (0.″85) and physical resolution (20-80 pc) measurements of the probability distribution function (PDF) of mid-infrared (mid-IR…

2024 The Astronomical Journal
JWST 14
Global Parameters of Eight W UMa-type Binary Systems
DOI: 10.1088/1538-3873/ad1ed3 Bibcode: 2024PASP..136b4201P

Poro, Atila; Paki, Ehsan; Michel, Raul +1 more

Multiband photometric investigations for eight binary systems of the W Ursae Majoris-type are presented. Six systems are presented for the first time to analyze their light curves. All the analyzed systems have a temperature below 5000 K and an orbital period of less than 0.28 days. We extracted primary and secondary minima from the ground-based o…

2024 Publications of the Astronomical Society of the Pacific
Gaia 14
IXPE observation of PKS 2155–304 reveals the most highly polarized blazar
DOI: 10.1051/0004-6361/202449166 Bibcode: 2024A&A...689A.119K

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +133 more

We report the X-ray polarization properties of the high-synchrotron-peaked (HSP) blazar PKS 2155‑304 based on observations with the Imaging X-ray Polarimetry Explorer (IXPE). We observed the source between Oct 27 and Nov 7, 2023. We also conducted an extensive contemporaneous multiwavelength (MW) campaign. We find that during the first half (T

2024 Astronomy and Astrophysics
XMM-Newton 14
Robust constraints on feebly interacting particles using XMM-Newton
DOI: 10.1103/PhysRevD.109.L101305 Bibcode: 2024PhRvD.109j1305L

Carenza, Pierluca; Balaji, Shyam; Luque, Pedro De la Torre

During galactic supernova (SN) explosions, a large amount of feebly interacting particles (FIPs) may be produced. In this work we analyze electrophilic FIPs with masses in the MeV-range that escape from SN and decay into electron-positron pairs, causing an exotic leptonic injection. This contribution adds up to known components, leading to an unex…

2024 Physical Review D
INTEGRAL XMM-Newton 14