Search Publications

A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii
DOI: 10.3847/1538-4357/ad4097 Bibcode: 2024ApJ...968...31W

Evans, A.; Starrfield, S.; Page, K. L. +2 more

A near-infrared spectrum of nova V1716 Scorpii (PNV J17224490-4137160), a recent bright ( Vmax=7.3 mag), Fermi-LAT detected γ-ray source, was mod…

2024 The Astrophysical Journal
Gaia 5
Are WASP-107-like Systems Consistent with High-eccentricity Migration?
DOI: 10.3847/1538-4357/ad5ffb Bibcode: 2024ApJ...972..159Y

Dai, Fei; Yu, Hang

WASP-107 b seems to be a poster child of the long-suspected high-eccentricity migration scenario. It is on a 5.7 day, polar orbit. The planet is Jupiter-like in radius but Neptune-like in mass with exceptionally low density. WASP-107 c is on a 1100 day, e = 0.28 orbit with at least Saturn mass. Planet b may still have a residual eccentricity of 0.…

2024 The Astrophysical Journal
Gaia 5
X-Rays from RS Ophiuchi's 2021 Eruption: Shocks In and Out of Ionization Equilibrium
DOI: 10.3847/1538-4357/ad1041 Bibcode: 2024ApJ...960..125I

Sokoloski, J. L.; Mukai, Koji; Islam, Nazma

The recurrent nova RS Ophiuchi (RS Oph) underwent its most recent eruption on 2021 August 8 and became the first nova to produce both detectable GeV and TeV emission. We used extensive X-ray monitoring with the Neutron Star Interior Composition Explorer Mission (NICER) to model the X-ray spectrum and probe the shock conditions throughout the 2021 …

2024 The Astrophysical Journal
Gaia 5
The Atmosphere of HD 149026b: Low Metal Enrichment and Weak Energy Transport
DOI: 10.3847/1538-4357/ad452d Bibcode: 2024ApJ...969...86G

Fortney, Jonathan J.; Batalha, Natasha E.; Mukherjee, Sagnick +1 more

Recent JWST eclipse spectra of the high-density hot Saturn HD 149026b between 2.35 and 5.08 µm have allowed for in-depth study of its atmosphere. To understand its atmospheric properties, we have created a grid of 1D radiative-convective–thermochemical–equilibrium atmosphere models and spectra with PICASO 3.0. In agreement with previous work…

2024 The Astrophysical Journal
JWST 5
Synthetic Gaia DR3 Surveys from the FIRE Cosmological Simulations of Milky Way-mass Galaxies
DOI: 10.3847/1538-4357/ad35ba Bibcode: 2024ApJ...966..108N

Sanderson, Robyn; Wetzel, Andrew; Necib, Lina +4 more

The third data release (DR3) of Gaia has provided a fivefold increase in the number of radial velocity measurements of stars, as well as a stark improvement in parallax and proper motion measurements. To help with studies that seek to test models and interpret Gaia DR3, we present nine Gaia synthetic surveys, based on three solar positions in thre…

2024 The Astrophysical Journal
Gaia 5
Protosolar D-to-H Abundance and One Part per Billion PH3 in the Coldest Brown Dwarf
DOI: 10.3847/2041-8213/ad9744 Bibcode: 2024ApJ...977L..49R

Fortney, Jonathan J.; Apai, Dániel; Marley, Mark +24 more

The coldest Y spectral type brown dwarfs are similar in mass and temperature to cool and warm (∼200–400 K) giant exoplanets. We can therefore use their atmospheres as proxies for planetary atmospheres, testing our understanding of physics and chemistry for these complex, cool worlds. At these cold temperatures, their atmospheres are cold enough fo…

2024 The Astrophysical Journal
JWST 5
eDIG-CHANGES. II. Project Design and Initial Results on NGC 3556
DOI: 10.3847/1538-4357/ad3cd8 Bibcode: 2024ApJ...967...78L

Bregman, Joel N.; Li, Hui; Martini, Paul +19 more

The extraplanar diffuse ionized gas (eDIG) represents ionized gases traced by optical/UV lines beyond the stellar extent of galaxies. We herein introduce a novel multislit narrow-band spectroscopy method to conduct spatially resolved spectroscopy of the eDIG around a sample of nearby edge-on disk galaxies (eDIG-CHANGES). In this paper, we introduc…

2024 The Astrophysical Journal
eHST 5
Kinematics of Supernova Remnants Using Multiepoch Maximum Likelihood Estimation: Chandra Observation of Cassiopeia A as an Example
DOI: 10.3847/1538-4357/ad739f Bibcode: 2024ApJ...974..245S

Sato, Toshiki; Yamada, Shinya; Sakai, Yusuke +2 more

Decadal changes in a nearby supernova remnant (SNR) were analyzed using a multiepoch maximum likelihood estimation (MLE) approach. To achieve greater accuracy in capturing the dynamics of SNRs, kinematic features and point-spread function effects were integrated into the MLE framework. Using Cassiopeia A as a representative example, data obtained …

2024 The Astrophysical Journal
JWST 5
Fast Outflows and Luminous He II Emission in Dwarf Galaxies with Active Galactic Nuclei (AGN)
DOI: 10.3847/1538-4357/ad2b63 Bibcode: 2024ApJ...965..152L

Tripp, Todd M.; Hamann, Fred; Veilleux, Sylvain +6 more

While stellar processes are believed to be the main source of feedback in dwarf galaxies, the accumulating discoveries of active galactic nuclei (AGN) in dwarf galaxies over recent years arouse the interest to also consider AGN feedback in them. Fast, AGN-driven outflows, a major mechanism of AGN feedback, have indeed been discovered in dwarf gala…

2024 The Astrophysical Journal
eHST 5
VLA FRAMEx. I. Wideband Radio Properties of the AGN in NGC 4388
DOI: 10.3847/1538-4357/ad11d4 Bibcode: 2024ApJ...961..230S

Fischer, Travis C.; Secrest, Nathan J.; Johnson, Megan C. +5 more

We present the first results from Karl G. Jansky Very Large Array (VLA) observations as a part of the Fundamental Reference Active Galactic Nucleus (AGN) Monitoring Experiment, a program to understand the relationship between AGN accretion physics and wavelength-dependent position as a function of time. With this VLA survey, we investigate the rad…

2024 The Astrophysical Journal
eHST 5