Search Publications

The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI-1246
DOI: 10.3847/1538-3881/ac69e5 Bibcode: 2022AJ....163..293T

Lester, Kathryn V.; Bieryla, Allyson; Latham, David W. +78 more

Multiplanet systems are valuable arenas for investigating exoplanet architectures and comparing planetary siblings. TOI-1246 is one such system, with a moderately bright K dwarf (V = 11.6, K = 9.9) and four transiting sub-Neptunes identified by TESS with orbital periods of 4.31, 5.90, 18.66, and 37.92 days. We collected 130 radial velocity observa…

2022 The Astronomical Journal
Gaia 12
Mid-ultraviolet Hubble Observations of Europa and the Global Surface Distribution of SO2
DOI: 10.3847/PSJ/ac69eb Bibcode: 2022PSJ.....3..129B

Alday, Juan; Roth, Lorenz; McGrath, Melissa A. +6 more

We present spatially resolved reflectance spectra of Europa's surface in the wavelength range of 210-315 nm obtained by the Hubble Space Telescope Imaging Spectrograph in 2018 and 2019. These data provide the first high-quality, near-global spectral observations of Europa from 210 to 240 nm. They show that the reflectance of Europa's leading, trai…

2022 The Planetary Science Journal
eHST 12
Accretion of a clumped wind from a red supergiant donor on to a magnetar is suggested by the analysis of the XMM-Newton and NuSTAR observations of the X-ray binary 3A 1954+319
DOI: 10.1093/mnras/stab3688 Bibcode: 2022MNRAS.510.4645B

Ducci, L.; Ferrigno, C.; Bozzo, E. +1 more

3A 1954+319 has been classified for a long time as a symbiotic X-ray binary, hosting a slowly rotating neutron star and an aged M red giant. Recently, this classification has been revised thanks to the discovery that the donor star is an M supergiant. This makes 3A 1954+319 a rare type of high-mass X-ray binary consisting of a neutron star and a r…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
The Far Ultra-violet Background
DOI: 10.1088/1538-3873/ac689e Bibcode: 2022PASP..134h4302K

Kulkarni, S. R.

The diffuse far-ultraviolet (FUV) background has received considerable attention from astronomers since the 1970s The initial impetus came from the hope of detecting UV radiation from the hot intergalactic medium. The central importance of the FUV background to the physics (heating and ionization) of the diffuse atomic phases motivated the next ge…

2022 Publications of the Astronomical Society of the Pacific
SOHO 12
An Elusive Population of Massive Disk Galaxies Hosting Double-lobed Radio-loud Active Galactic Nuclei
DOI: 10.3847/1538-4357/ac9cd5 Bibcode: 2022ApJ...941...95W

Ho, Luis C.; Zhuang, Ming-Yang; Wu, Zihao

It is commonly accepted that radio-loud active galactic nuclei are hosted exclusively by giant elliptical galaxies. We analyze high-resolution optical Hubble Space Telescope images of a sample of radio galaxies with extended double-lobed structures associated with disk-like optical counterparts. After systematically evaluating the probability of c…

2022 The Astrophysical Journal
eHST 12
The Extended Field-aligned Suprathermal Proton Beam and Long-lasting Trapped Energetic Particle Population Observed Upstream of a Transient Interplanetary Shock
DOI: 10.3847/1538-4357/ac3c47 Bibcode: 2022ApJ...925..198L

Lario, D.; Jian, L. K.; Wilson, L. B., III +3 more

The properties of the suprathermal particle distributions observed upstream of interplanetary shocks depend not only on the properties of the shocks but also on the transport conditions encountered by the particles as they propagate away from the shocks. The confinement of particles in close proximity to the shocks, as well as particle scattering …

2022 The Astrophysical Journal
SOHO 12
pterodactyls: A Tool to Uniformly Search and Vet for Young Transiting Planets in TESS Primary Mission Photometry
DOI: 10.3847/1538-3881/ac7b29 Bibcode: 2022AJ....164...78F

Pascucci, Ilaria; Ciardi, David R.; Giacalone, Steven +8 more

Kepler's short-period exoplanet population has revealed evolutionary features such as the Radius Valley and the Hot Neptune desert that are likely sculpted by atmospheric loss over time. These findings suggest that the primordial planet population is different from the Gyr-old Kepler population, and motivates exoplanet searches around young stars.…

2022 The Astronomical Journal
Gaia 12
Atmospheric Characterization of Hot Jupiter CoRoT-1 b Using the Wide Field Camera 3 on the Hubble Space Telescope
DOI: 10.3847/1538-3881/ac6cdb Bibcode: 2022AJ....164...19G

Deming, Drake; Zhou, Yifan; Schlawin, Everett +3 more

Exoplanet CoRoT-1 b is intriguing because we predict it to be a transitional planet between hot Jupiters (equilibrium temperatures ~1500 K) and ultrahot Jupiters (equilibrium temperatures >2000 K). In 2012, observations of CoRoT-1 b included one primary transit and three secondary eclipses with the Hubble Space Telescope (HST) Wide Field Camera…

2022 The Astronomical Journal
eHST 12
A 6D view of stellar shells
DOI: 10.1093/mnras/stab3361 Bibcode: 2022MNRAS.510..230D

Evans, N. W.; Vasiliev, E.; Dong-Páez, C. A.

Stellar shells are low surface brightness features, created during nearly head-on galaxy mergers from the debris of the tidally disrupted satellite. Here, we investigate the formation and evolution mechanism of shells in six dimensions (3D positions and velocities). We propose a new description in action-angle coordinates which condenses the seemi…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 12
Manifestation of Gravitational Settling in Coronal Mass Ejections Measured in the Heliosphere
DOI: 10.3847/1538-4357/ac8873 Bibcode: 2022ApJ...936...83R

Reeves, Katharine K.; Landi, Enrico; Raymond, John C. +4 more

Elemental composition in the solar wind reflects the fractionation processes at the Sun. In coronal mass ejections (CMEs) measured in the heliosphere, the elemental composition can vary between plasma of high and low ionization states as indicated by the average Fe charge state, <QFe>. It is found that CMEs with higher ionized pla…

2022 The Astrophysical Journal
SOHO 12