Search Publications

AT2018fyk: Candidate Tidal Disruption Event by a (Super)Massive Black Hole Binary
DOI: 10.3847/1538-4357/ad4da3 Bibcode: 2024ApJ...970..116W

Wevers, T.; Li, D.; Kara, E. +8 more

The tidal disruption event (TDE) AT2018fyk has unusual X-ray, UV, and optical light curves that decay over the first ∼600 days, rebrighten, and decay again around 1200 days. We explain this behavior as a one-off TDE associated with a massive black hole (BH) binary. The sharp drop-offs from t ‑5/3 power laws at around 600 days naturally …

2024 The Astrophysical Journal
XMM-Newton eHST 6
Chemical Diagnostics to Unveil Environments Enriched by First Stars
DOI: 10.3847/2041-8213/ad46fa Bibcode: 2024ApJ...967L..22V

Cupani, Guido; D'Odorico, Valentina; Becker, George D. +2 more

Unveiling the chemical fingerprints of the first (Population III, hereafter Pop III) stars is crucial for indirectly studying their properties and probing their massive nature. In particular, very massive Pop III stars explode as energetic pair-instability supernovae (PISNe), allowing their chemical products to escape in the diffuse medium around …

2024 The Astrophysical Journal
JWST 6
Dracula's Chivito: Discovery of a Large Edge-on Protoplanetary Disk with Pan-STARRS
DOI: 10.3847/2041-8213/ad43e3 Bibcode: 2024ApJ...967L...3B

Drake, Jeremy J.; Bayyari, Ammar; Russell, Ray W. +6 more

We report the serendipitous discovery of a large edge-on protoplanetary disk in Pan-STARRS (PS1) images. PS1 has five broadband filters designated as g P1, r P1, i P1, z P1, and y P1 with mean wavelengths 4866, 6215, 7545, 8679, and 9633 Å, respectively. The disk's apparent size in the PS1 ima…

2024 The Astrophysical Journal
AKARI Gaia 6
The Next Step in Galaxy Cluster Strong Lensing: Modeling the Surface Brightness of Multiply Imaged Sources
DOI: 10.3847/1538-4357/ad8343 Bibcode: 2024ApJ...976..110A

Acebron, Ana; Nonino, Mario; Grillo, Claudio +12 more

Overcoming both modeling and computational challenges, we present, for the first time, the extended surface-brightness distribution model of a strongly lensed source in a complex galaxy-cluster-scale system. We exploit the high-resolution Hubble Space Telescope (HST) imaging and extensive Multi Unit Spectroscopic Explorer spectroscopy to build an …

2024 The Astrophysical Journal
eHST 6
The Green Monster Hiding in Front of Cas A: JWST Reveals a Dense and Dusty Circumstellar Structure Pockmarked by Ejecta Interactions
DOI: 10.3847/2041-8213/ad855d Bibcode: 2024ApJ...976L...4D

Temim, Tea; Rest, Armin; Blair, William P. +27 more

JWST observations of the young Galactic supernova remnant Cassiopeia A revealed an unexpected structure seen as a green emission feature in colored composite MIRI F1130W and F1280W images—hence dubbed the Green Monster—that stretches across the central parts of the remnant in projection. Combining the kinematic information from NIRSpec and the MIR…

2024 The Astrophysical Journal
eHST JWST 6
X-Ray and Multiwavelength Polarization of Mrk 501 from 2022 to 2023
DOI: 10.3847/1538-4357/ad63a1 Bibcode: 2024ApJ...974...50C

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +143 more

We present multiwavelength polarization measurements of the luminous blazar Mrk 501 over a 14 month period. The 2–8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100 ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR,…

2024 The Astrophysical Journal
XMM-Newton 6
JWST Mid-infrared Spectroscopy Resolves Gas, Dust, and Ice in Young Stellar Objects in the Large Magellanic Cloud
DOI: 10.3847/1538-4357/ad18bc Bibcode: 2024ApJ...963...94N

Hirschauer, Alec S.; Lenkić, Laura; Meixner, Margaret +9 more

In this work, we present spectra of 11 young stellar objects (YSOs) taken with the Mid-Infrared Instrument / Medium Resolution Spectroscopy (MRS) instrument on board the James Webb Space Telescope (JWST). The YSOs are located in the N79 region of the Large Magellanic Cloud (LMC), an active star-forming region with hundreds of Spitzer- and Herschel…

2024 The Astrophysical Journal
JWST 6
Merging Signatures in an Offset Lyman Continuum Emitter at Redshift 3.8
DOI: 10.3847/1538-4357/ad75ff Bibcode: 2024ApJ...975...53Y

Zheng, Zhen-Ya; Cheng, Cheng; Yuan, Fang-Ting +3 more

Lyman continuum (LyC) emitters at z > 3 provide critical samples for studying the contribution of galaxies to the ionizing background in the epoch of reionization. We collect a sample of z > 3 LyC emitters, a dominant fraction (∼60%–70%) of which show spatial offsets between LyC emission and the nonionizing continuum. From this sample, espec…

2024 The Astrophysical Journal
eHST JWST 6
Comparative Analysis of Type III Radio Bursts and Solar Flares: Spatial Localization and Correlation with Solar Flare Intensity
DOI: 10.3847/1538-4357/ad12ba Bibcode: 2024ApJ...961...88K

Maksimovic, Milan; Szabo, Adam; Bale, Stuart D. +8 more

We present a comprehensive study of type III radio bursts and their association with solar flares of magnitude M1.0 and larger, as observed by four widely separated spacecraft (Parker Solar Probe, Solar Orbiter, STEREO-A, and Wind). Our main focus is the introduction and validation of two methods for localizing radio bursts using the available mul…

2024 The Astrophysical Journal
SolarOrbiter Ulysses 6
JWST/NIRCam Paβ Narrowband Imaging Reveals Ordinary Dust Extinction for Hα Emitters within the Spiderweb Protocluster at z = 2.16
DOI: 10.3847/1538-4357/ad8156 Bibcode: 2024ApJ...977...74P

Pérez-González, Pablo G.; Koyama, Yusei; Kodama, Tadayuki +7 more

We combine JWST/NIRCam and Subaru/MOIRCS dual Paβ+Hα narrowband imaging to trace the dust attenuation and the star formation activities of a sample of 43 Hα emitters at the core of one of the most massive and best-studied clusters in formation at the cosmic noon: the Spiderweb protocluster at z = 2.16. We find that most Hα emitters display Paβ/Hα …

2024 The Astrophysical Journal
JWST 6