Search Publications

Quantifying the Transit Light Source Effect: Measurements of Spot Temperature and Coverage on the Photosphere of AU Microscopii with High-resolution Spectroscopy and Multicolor Photometry
DOI: 10.3847/1538-4357/ad0bed Bibcode: 2024ApJ...962...97W

Wakeford, Hannah R.; Mann, Andrew W.; Plavchan, Peter +5 more

AU Microscopii (AU Mic) is an active 24 ± 3 Myr pre-main-sequence M dwarf in the stellar neighborhood (d = 9.7 pc) with a rotation period of 4.86 days. The two transiting planets orbiting AU Mic, AU Mic b and c, are warm sub-Neptunes on 8.5 and 18.9 day periods and are targets of interest for atmospheric observations of young planets. Here we stud…

2024 The Astrophysical Journal
Gaia eHST 4
Astroparticles from X-Ray Binary Coronae
DOI: 10.3847/2041-8213/ad887b Bibcode: 2024ApJ...975L..35F

Gallagher, John S.; Fang, K.; Halzen, Francis +1 more

The recent observation of high-energy neutrinos from the Galactic plane implies an abundant population of hadronic cosmic-ray sources in the Milky Way. We explore the role of the coronae of accreting stellar-mass black holes as such astroparticle emitters. We show that the particle acceleration and interaction timescales in the coronal region are …

2024 The Astrophysical Journal
INTEGRAL 4
Filament Eruption from Active Region 13283 Leading to a Fast Halo-CME and an Intense Geomagnetic Storm on 2023 April 23
DOI: 10.3847/1538-4357/ad1662 Bibcode: 2024ApJ...961..199V

Vemareddy, P.

Using multi-instrument and multiwavelength observations, we studied a coronal mass ejection (CME) that led to an intense geomagnetic storm on 2023 April 23. The eruption occurred on April 21 in solar active region (AR) 13283 near the disk center. The AR was in its decay stage, with fragmented polarities and a preexisting long filament channel a fe…

2024 The Astrophysical Journal
SOHO 4
Insights into the Galactic Bulge Chemodynamical Properties from Gaia Data Release 3
DOI: 10.3847/1538-4357/ad38ba Bibcode: 2024ApJ...967....5L

Marinacci, Federico; Fragkoudi, Francesca; Shen, Juntai +4 more

We explore the chemodynamical properties of the Galaxy in the azimuthal velocity V ϕ and metallicity [Fe/H] space using red giant stars from Gaia Data Release 3. The row-normalized V ϕ –[Fe/H] maps form a coherent sequence from the bulge to the outer disk, clearly revealing the thin/thick disk and the Splash. The metal-ric…

2024 The Astrophysical Journal
Gaia 4
Trojan Globular Clusters: Radial Migration via Trapping in Bar Resonances
DOI: 10.3847/2041-8213/ad60c8 Bibcode: 2024ApJ...971L...4D

Belokurov, Vasily; Monty, Stephanie; Evans, N. Wyn +1 more

We search for globular clusters (GCs) trapped in resonances with the bar of the Milky Way (MW). By integrating their orbits in a potential with a decelerating bar, we select 10 whose orbits are significantly changed by its presence. Most of these are trapped in the corotation resonance, including M22 and 47 Tuc. The decelerating bar is capable of …

2024 The Astrophysical Journal
Gaia 4
Substructures within Substructures in the Complex Postmerging System A514 Unveiled by High-resolution Magellan/Megacam Weak Lensing
DOI: 10.3847/1538-4357/ad65dc Bibcode: 2024ApJ...973...79A

Jee, M. James; Lee, Wonki; ZuHone, John +2 more

Abell 514 (A514) at z = 0.071 is an intriguing merging system exhibiting highly elongated (∼1 Mpc) X-ray features and three large-scale (300 ∼ 500 kpc) bent radio jets. To dissect this system with its multiwavelength data, it is critical to robustly identify and quantify its dark matter substructures. We present a weak-lensing analysis of A514 usi…

2024 The Astrophysical Journal
XMM-Newton 4
Interplanetary Type IV Solar Radio Bursts: A Comprehensive Catalog and Statistical Results
DOI: 10.3847/1538-4357/ad5315 Bibcode: 2024ApJ...971...86M

Mohan, Atul; Gopalswamy, Nat; Kumari, Anshu +2 more

Decameter hectometric (DH; 1–14 MHz) type IV radio bursts are produced by flare-accelerated electrons trapped in postflare loops or the moving magnetic structures associated with the coronal mass ejections (CMEs). From a space weather perspective, it is important to systematically compile these bursts, explore their spectrotemporal characteristics…

2024 The Astrophysical Journal
SOHO 4
HST Proper Motion of Andromeda III. Another Satellite Coorbiting the M31 Satellite Plane
DOI: 10.3847/1538-4357/ad7b10 Bibcode: 2024ApJ...975..138C

Kozhurina-Platais, Vera; Casetti-Dinescu, Dana I.; Girard, Terrence M. +5 more

We measure the absolute proper motion of Andromeda III (And III) using Advanced Camera for Surveys/Wide Field Channel and WFPC2 exposures spanning an unprecedented 22 yr time baseline. The WFPC2 exposures have been processed using a deep-learning centering procedure recently developed as well as an improved astrometric calibration of the camera. T…

2024 The Astrophysical Journal
Gaia eHST 4
An Empirical Framework Characterizing the Metallicity and Star-formation History Dependence of X-Ray Binary Population Formation and Emission in Galaxies
DOI: 10.3847/1538-4357/ad8de7 Bibcode: 2024ApJ...977..189L

Greene, Jenny E.; Oskinova, Lidia; Basu-Zych, Antara +12 more

We present a new empirical framework modeling the metallicity and star formation history (SFH) dependence of X-ray luminous (L ≳ 1036 erg s‑1) point-source population X-ray luminosity functions (XLFs) in normal galaxies. We expect that the X-ray point-source populations are dominated by X-ray binaries (XRBs), with contributio…

2024 The Astrophysical Journal
Herschel eHST JWST 4
A New Dissociative Galaxy Cluster Merger: RM J150822.0+575515.2
DOI: 10.3847/1538-4357/ad3249 Bibcode: 2024ApJ...966...49S

Finner, Kyle; Wittman, David; Stancioli, Rodrigo +1 more

Galaxy cluster mergers that exhibit clear dissociation between their dark matter, intracluster gas, and stellar components are great laboratories for probing dark matter properties. Mergers that are binary and in the plane of the sky have the additional advantage of being simpler to model, allowing for a better understanding of the merger dynamics…

2024 The Astrophysical Journal
XMM-Newton eHST 4