Search Publications

Characterization of Monosubstituted Benzene Ices
DOI: 10.3847/1538-4357/ad6c3b Bibcode: 2024ApJ...974..313P

Öberg, Karin I.; Piacentino, Elettra L.; Balkanski, Aurelia +1 more

Aromatic structures are fundamental for key biological molecules such as RNA and metabolites and the abundances of aromatic molecules on young planets are therefore of high interest. Recent detections of benzonitrile and other aromatic compounds in interstellar clouds and comets have revealed a rich aromatic astrochemistry. In the cold phases of s…

2024 The Astrophysical Journal
JWST 2
Nonthermal Observations of a Flare Loop-top Using IRIS Fe XXI: Implications for Turbulence and Electron Acceleration
DOI: 10.3847/1538-4357/ad64ca Bibcode: 2024ApJ...973...96A

Polito, Vanessa; Yu, Sijie; Hayes, Laura A. +2 more

The excess broadening of high-temperature spectral lines, long observed near the tops of flare arcades, is widely considered to result from magnetohydrodynamic turbulence. According to different theories, plasma turbulence is also believed to be a candidate mechanism for particle acceleration during solar flares. However, the degree to which this …

2024 The Astrophysical Journal
IRIS SolarOrbiter 2
Observations of Nonthermal Velocities and Comparisons with an Alfvén Wave Turbulence Model in Solar Active Regions
DOI: 10.3847/1538-4357/ad434a Bibcode: 2024ApJ...968....7A

Hahn, M.; Savin, D. W.; Brooks, D. H. +3 more

We present a study of spectral line width measurements from the Extreme-ultraviolet Imaging Spectrometer on Hinode. We used spectral line profiles of Fe XVI 262.984 Å, Fe XIV 264.787 Å, Fe XIV 270.519 Å, Fe XIV 274.203 Å, and Fe XV 284.160 Å, and studied 11 active regions. Previous studies of spectral line widths have shown that in hot loops in th…

2024 The Astrophysical Journal
Hinode 2
JADES: Spectroscopic Confirmation and Proper Motion for a T-Dwarf at 2 kpc
DOI: 10.3847/1538-4357/ad76a7 Bibcode: 2024ApJ...975...31H

Carniani, Stefano; D'Eugenio, Francesco; Bunker, Andrew J. +15 more

Large area observations of extragalactic deep fields with the James Webb Space Telescope (JWST) have provided a wealth of candidate low-mass L- and T-class brown dwarfs. The existence of these sources, which are at derived distances of hundreds of parsecs to several kiloparsecs from the Sun, has strong implications for the low-mass end of the stel…

2024 The Astrophysical Journal
JWST 2
Multiwavelength Observations of Sgr A*. II. 2019 July 21 and 26
DOI: 10.3847/1538-4357/ad5332 Bibcode: 2024ApJ...971...52M

Smith, Howard A.; Fazio, Giovanni G.; Bushouse, Howard +6 more

We report on the final two days of a multiwavelength campaign of Sgr A* observing in the radio, submillimeter, infrared (IR), and X-ray bands in 2019 July. Sgr A* was remarkably active, showing multiple flaring events across the electromagnetic spectrum. We detect a transient ∼35 minute periodicity feature in Spitzer light curves on 2019 July 21. …

2024 The Astrophysical Journal
eHST 2
A Morphokinematic Study of the Enigmatic Emission Nebula NGC 6164/5 Surrounding the Magnetic O-type Star HD 148937
DOI: 10.3847/1538-4357/ad12c4 Bibcode: 2024ApJ...961...72L

Lim, Beomdu; Nazé, Yaël; Chang, Seok-Jun +1 more

HD 148937 is a peculiar massive star (Of?p) with a strong magnetic field (1 kG). The hourglass-shaped emission nebula NGC 6164/5 surrounds this star. This nebula is presumed to originate from episodic mass-loss events of the central O-type star, but the detailed formation mechanism is not yet well understood. Grasping its three-dimensional structu…

2024 The Astrophysical Journal
Gaia 2
A Complete 16 µm Selected Galaxy Sample at z ∼ 1. II. Morphological Analysis
DOI: 10.3847/1538-4357/ad4a73 Bibcode: 2024ApJ...970...29L

Cheng, Cheng; Huang, Jia-Sheng; Dai, Y. Sophia +2 more

We present a morphological analysis of the 16 µm flux-density-limited galaxy sample at 0.8 < z < 1.3 from Huang et al. (2021). At the targeted redshift, the 16 µm emission corresponds to the polycyclic aromatic hydrocarbon feature from intense star formation, or dust heated by active galactic nuclei (AGN). Our sample of 479 galax…

2024 The Astrophysical Journal
eHST 2
Direct Observational Evidence of Multi-epoch Massive Star Formation in G24.47+0.49
DOI: 10.3847/2041-8213/ad6144 Bibcode: 2024ApJ...970L..40S

Sanhueza, Patricio; Tej, Anandmayee; Hwang, Jihye +19 more

Using new continuum and molecular line data from the Atacama Large Millimeter/submillimeter Array Three-millimeter Observations of Massive Star-forming Regions (ATOMS) survey and archival Very Large Array, 4.86 GHz data, we present direct observational evidence of hierarchical triggering relating three epochs of massive star formation in a ringlik…

2024 The Astrophysical Journal
Herschel 2
Relative Occurrence Rate between Hot and Cold Jupiters as an Indicator to Probe Planet Migration
DOI: 10.3847/1538-4357/ad3deb Bibcode: 2024ApJ...967...74G

Fulton, Benjamin J.; Gan, Tianjun; Mao, Shude +4 more

We propose a second-order statistic parameter ɛ, the relative occurrence rate between hot Jupiters (HJs) and cold Jupiters (CJs) (ɛ = η HJCJ), to probe the migration of gas giants. Since the planet occurrence rate is the combined outcome of the formation and migration processes, a joint analysis of HJ and CJ frequency may …

2024 The Astrophysical Journal
Gaia 2
Quasiperiodic Oscillations of Flare Loops and Slipping Motion of Ribbon Substructures during a C-class Flare
DOI: 10.3847/1538-4357/ad5e69 Bibcode: 2024ApJ...972..122Z

Li, Ting; Ye, Jing; Zhang, Yining

Quasiperiodic oscillations in solar-flaring emission have been observed over the past few decades. To date, the underpinning processes resulting in the quasiperiodic oscillations remain unknown. In this paper, we report a unique event that exhibits both the long-duration quasiperiodic intensity oscillations of flare loops and the quasiperiodic sli…

2024 The Astrophysical Journal
IRIS 2