Search Publications

On the Orbit of the Binary Brown Dwarf Companion GL229 Ba and Bb
DOI: 10.3847/1538-3881/adb4f2 Bibcode: 2025AJ....169..193T

Henning, Thomas; Mérand, Antoine; Johnstone, Doug +21 more

The companion GL229B was recently resolved by Xuan et al. as a tight binary of two brown dwarfs (Ba and Bb) through VLTI-GRAVITY interferometry and Very Large Telescope-CRIRES+ radial velocity (RV) measurements. Here, we present Bayesian models of the interferometric and RV data in additional detail, along with an updated outer orbit of the brown …

2025 The Astronomical Journal
Gaia Hipparcos 0
Discoveries and Properties of EL CVn–type Binaries in the TESS Survey
DOI: 10.3847/1538-4357/ad9b9c Bibcode: 2025ApJ...979..108X

Han, Zhanwen; Chen, Xuefei; Li, Zhenwei +5 more

EL CVn–type systems represent a rare evolutionary stage in binary star evolution, providing ideal laboratories for investigating stable mass-transfer processes and the formation of extremely low-mass white dwarfs (ELM WDs). The Transiting Exoplanet Survey Satellite (TESS) has delivered an extensive collection of high-precision time-domain photomet…

2025 The Astrophysical Journal
Gaia 0
ALMA Observations of Peculiar Embedded Icy Objects
DOI: 10.3847/1538-4357/ada4ad Bibcode: 2025ApJ...981...49S

Onaka, Takashi; Sakon, Itsuki; Shimonishi, Takashi

We report the results of molecular line observations with the Atacama Large Millimeter/submillimeter Array (ALMA) toward two peculiar icy objects, which were discovered serendipitously by infrared spectroscopic survey of the Galactic plane with the AKARI satellite. Previous infrared observations have reported that both objects show deep ice and du…

2025 The Astrophysical Journal
AKARI 0
Eight New Candidate Multiplanet Systems among TESS Objects of Interest
DOI: 10.3847/1538-3881/ad9a6c Bibcode: 2025AJ....169...91M

Kunimoto, Michelle; Munavar Hussain, Mohamed Jassim

We present a search of the TESS Object of Interest (TOI) Catalog for new multiplanet systems. We perform a Box Least Squares search on light curves prepared by the Quick-Look Pipeline to recover known candidates and perform a targeted search for additional candidates in each system. Following vetting and manual inspection, we present eight new pla…

2025 The Astronomical Journal
Gaia 0
Planetary Mass Determinations from a Simplified Photodynamical Model—Application to the Complete Kepler Dataset
DOI: 10.3847/1538-3881/ad91a7 Bibcode: 2025AJ....169...90O

Aharonson, Oded; Ofir, Aviv; Yoffe, Gideon

We use PyDynamicaLC, a model using the least number of—and the least correlated—degrees of freedom needed to derive a photodynamical model, to describe some of the smallest—and lowest-transit-timing-variation-amplitude—of the Kepler planets. We successfully analyze 64 systems containing 218 planets, for 88 of which we were able to determine signif…

2025 The Astronomical Journal
Gaia 0
Spectra of standing kink waves in loops and the effects of the lower solar atmosphere
DOI: 10.1051/0004-6361/202452399 Bibcode: 2025A&A...693A.261K

Gao, Yuhang; Van Doorsselaere, Tom; Lim, Daye +1 more

Context. Understanding the effects of the lower solar atmosphere on the spectrum of standing kink oscillations of coronal loops, in both the decaying and decayless regime, is essential for developing more advanced tools for coronal seismology. Aims. We aim to reveal the effects of the chromosphere on the spatial profiles and frequencies of the sta…

2025 Astronomy and Astrophysics
SolarOrbiter 0
The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.4 and 0.6
DOI: 10.1093/mnras/stae2498 Bibcode: 2025MNRAS.536..518P

McHardy, I.; Page, M. J.; Seymour, N. +7 more

We combine ultraviolet imaging of the $13^{H}$ survey field, taken with the XMM-Newton Optical Monitor telescope (XMM-OM) and the Neil Gehrels Swift Observatory Ultraviolet and Optical Telescope (UVOT) in the UVM2 band, to measure rest-frame ultraviolet 1500 Å lumin…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
The Surprising Long-Term Evolution of the ULXP NGC 7793 P13
DOI: 10.1002/asna.20240106 Bibcode: 2025AN....34640106F

Fürst, Felix; Walton, Dominic J.; Brightman, Murray +2 more

The ultra-luminous x-ray pulsar (ULXP) NGC 7793 P13 has been regularly monitored with XMM-Newton, NuSTAR, and Swift for the last 8 years. Here, we present the latest results of this monitoring campaign with respect to the pulse period evolution and spectral variability. We find that since the source recovered from an x-ray low state in 2020–2022 t…

2025 Astronomische Nachrichten
XMM-Newton 0
Hinode/EIS Observation of the Alfvénic Fluctuations in the Quiet Sun
DOI: 10.3847/1538-4357/adb9e5 Bibcode: 2025ApJ...982...59T

Young, Peter R.; Morton, Richard; Tajfirouze, Edris

Alfvénic fluctuations in the corona are regularly observed in EUV imaging and infrared spectroscopic data. We report here on the Doppler velocity fluctuations within the data from the Extreme-Ultraviolet Imaging Spectrometer (EIS) on board Hinode. The capabilities of EIS provide an opportunity to detect fluctuations in the solar atmosphere and con…

2025 The Astrophysical Journal
Hinode 0
Insights into the origins of Phobos and Deimos based on a spectral comparison with small bodies and Martian materials
DOI: 10.1051/0004-6361/202453080 Bibcode: 2025A&A...694A.304W

Fornasier, S.; Doressoundiram, A.; Mahlke, M. +4 more

Context. The origins of Phobos and Deimos are highly debated, and several distinct hypotheses have been put forth. The two most widely accepted theories are that (1) the two moons were created by a giant impact in analogy to the Earth-Moon system, whereby a debris disk was formed that then formed the two moons by accretion; and that (2) the moons …

2025 Astronomy and Astrophysics
AKARI Gaia 0