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
Effect of temperature on measurement of fundamental constants using white dwarfs in Gaia-EDR3 survey
DOI: 10.1093/mnras/stad3123 Bibcode: 2024MNRAS.527..232U

Uniyal, Akhil; Kalita, Surajit; Chakrabarti, Sayan

Fundamental constants are crucial for comprehending physical mechanisms, but their measurements contain uncertainties due to experimental limitations. We investigate the impact of system temperature on these uncertainties using nearby white dwarfs observed in the Gaia Early Data Release 3 (EDR3) survey. Using the structures of these white dwarfs, …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
X-ray detection of the most extreme star-forming galaxies at the cosmic noon via strong lensing
DOI: 10.1093/mnras/stad3827 Bibcode: 2024MNRAS.52710584W

Frye, Brenda L.; Yun, Min S.; Liu, Daizhong +11 more

Hyperluminous infrared galaxies (HyLIRGs) are the most extreme star-forming systems observed in the early Universe, and their properties still elude comprehensive understanding. We have undertaken a large XMM-Newton observing programme to probe the total accreting black hole population in three HyLIRGs at z = 2.12, 3.25, and 3.55, gravitationally …

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 2
Particle acceleration at the bow shock of runaway star LS 2355: non-thermal radio emission but no γ-ray counterpart
DOI: 10.1093/mnras/stae1622 Bibcode: 2024MNRAS.532.2920V

Motta, S.; van den Eijnden, J.; Mohamed, S. +3 more

Massive stars that travel at supersonic speeds can create bow shocks as their stellar winds interact with the surrounding interstellar medium (ISM). These bow shocks - prominent sites for mechanical feedback of individual massive stars - are predominantly observed in the infrared (IR) band. Confirmed high-energy emission from stellar bow shocks ha…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Unraveling the kinematics of IZw18: A detailed study of ionized gas with MEGARA/GTC
DOI: 10.1051/0004-6361/202449606 Bibcode: 2024A&A...687A..77A

Kehrig, C.; Pérez-Montero, E.; Vílchez, J. M. +6 more

This study offers an in-depth analysis of the kinematic behavior of ionized gas in IZw18, a galaxy notable for its extremely low metallicity and close proximity, utilizing data from MEGARA/GTC. We explored the structure and dynamics of the galaxy through Hα line profiles, applying single and double Gaussian component fittings to create detailed ma…

2024 Astronomy and Astrophysics
eHST 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