Search Publications

Slow Rotation for the Super-puff Planet Kepler-51d
DOI: 10.3847/2041-8213/ad91ae Bibcode: 2024ApJ...977L...1L

Winn, Joshua N.; Lammers, Caleb

Super-puffs are low-density planets of unknown origin and composition. If they form by accreting nebular gas through a circumplanetary disk, one might expect super-puffs to be spinning quickly. Here, we derive upper limits on the rotational oblateness of the super-puff Kepler-51d, based on precise transit observations with the NIRSpec instrument o…

2024 The Astrophysical Journal
JWST 5
Searching for GEMS: Characterizing Six Giant Planets Around Cool Dwarfs
DOI: 10.3847/1538-3881/ad7796 Bibcode: 2024AJ....168..235K

Kobulnicky, Henry A.; Vanderburg, Andrew; Kowalski, Adam F. +42 more

Transiting giant exoplanets around M-dwarf stars (GEMS) are rare, owing to the low-mass host stars. However, the all-sky coverage of TESS has enabled the detection of an increasingly large number of them to enable statistical surveys like the Searching for GEMS survey. As part of this endeavor, we describe the observations of six transiting giant …

2024 The Astronomical Journal
Gaia 5
Radial Wave in the Galactic Disk: New Clues to Discriminate Different Perturbations
DOI: 10.3847/1538-4357/ad7b0e Bibcode: 2024ApJ...975..292C

Antoja, Teresa; Schönrich, Ralph; Li, Zhao-Yu +1 more

Decoding the key dynamical processes that shape the Galactic disk structure is crucial for reconstructing the Milky Way's evolution history. The second Gaia data release unveils a novel wave pattern in the L Z ‑<V R > space, but its formation mechanism remains elusive due to the intricate nature of involved perturbati…

2024 The Astrophysical Journal
Gaia 5
Evidence for transient morning water frost deposits on the Tharsis volcanoes of Mars
DOI: 10.1038/s41561-024-01457-7 Bibcode: 2024NatGe..17..608V

Vandaele, A. C.; Daerden, F.; Ristic, B. +27 more

The present-day water cycle on Mars has implications for habitability and future human exploration. Water ice clouds and water vapour have been detected above the Tharsis volcanic province, suggesting the active exchange of water between regolith and atmosphere. Here we report observational evidence for extensive transient morning frost deposits o…

2024 Nature Geoscience
ExoMars-16 MEx 5
eROSITA studies of the Carina nebula
DOI: 10.1051/0004-6361/202347154 Bibcode: 2024A&A...682A.172S

Sasaki, Manami; Pühlhofer, Gerd; Tsuge, Kisetsu +4 more

Context. During the first four all-sky surveys eRASS:4, which was carried out from December 2019 to 2021, the extended Roentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spektrum-Roentgen-Gamma (Spektr-RG, SRG) observed the Galactic H II region, the Carina nebula.
Aims: We analysed the eRASS:4 data to study the distributio…

2024 Astronomy and Astrophysics
AKARI 5
Benchmarking the IRDC G351.77-0.53: Gaia DR3 distance, mass distribution, and star formation content
DOI: 10.1093/mnras/stae631 Bibcode: 2024MNRAS.529.2220R

Megeath, S. T.; Xu, Fengwei; Stutz, A. M. +4 more

While intensively studied, it remains unclear how the star formation (SF) in infrared dark clouds (IRDCs) compares to that of nearby clouds. We study G351.77-0.53 (henceforth G351), a cluster-forming filamentary IRDC. We begin by characterizing its young stellar object (YSO) content. Based on the average parallax of likely members, we obtain a Gai…

2024 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 5
The Orbit and Companion of PSR J1622-0315: Variable Asymmetry and a Massive Neutron Star
DOI: 10.3847/1538-4357/ad6314 Bibcode: 2024ApJ...973..121S

Kennedy, Mark R.; Turchetta, Marco; Sen, Bidisha +6 more

The companion to PSR J1622-0315, one of the most compact known redback millisecond pulsars, shows extremely low irradiation despite its short orbital period. We model this system to determine the binary parameters, combining optical observations from the New Technology Telescope in 2017 and the Nordic Optical Telescope in 2022 with the binary mode…

2024 The Astrophysical Journal
Gaia 5
An X-ray high-frequency quasi-periodic oscillation in NGC 1365
DOI: 10.1051/0004-6361/202450875 Bibcode: 2024A&A...691A...7Y

Zhang, P.; Chang, Z.; Yan, J. Z. +4 more

This study presents the detection of a high-frequency quasi-periodic oscillation (QPO) in the Seyfert galaxy NGC 1365 based on observational data obtained by XMM-Newton in January 2004. Utilizing the weighted wavelet Z-transform (WWZ) and Lomb-Scargle periodogram (LSP) methods, a QPO signal is identified at a frequency of 2.19 × 10‑4 Hz…

2024 Astronomy and Astrophysics
XMM-Newton 5
Assessing the Performance of the ADAPT and AFT Flux Transport Models Using In Situ Measurements from Multiple Satellites
DOI: 10.3847/1538-4357/ad25f1 Bibcode: 2024ApJ...964..188K

Warren, Harry P.; Linton, Mark G.; Ugarte-Urra, Ignacio +7 more

The launches of Parker Solar Probe (Parker) and Solar Orbiter (SolO) are enabling a new era of solar wind studies that track the solar wind from its origin at the photosphere, through the corona, to multiple vantage points in the inner heliosphere. A key ingredient for these models is the input photospheric magnetic field map that provides the bou…

2024 The Astrophysical Journal
Hinode SolarOrbiter 5
VaDAR: Varstrometry for Dual AGN Using Radio Interferometry
DOI: 10.3847/1538-4357/ad0ed0 Bibcode: 2024ApJ...961..233S

Nyland, Kristina; Clarke, Tracy E.; Satyapal, Shobita +5 more

Binary and dual active galactic nuclei (AGNs) are an important observational tool for studying the formation and dynamical evolution of galaxies and supermassive black holes. An entirely new method for identifying possible AGN pairs makes use of the exquisite positional accuracy of Gaia to detect astrometrically variable quasars, in tandem with th…

2024 The Astrophysical Journal
Gaia eHST 5