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New Coronae and Stellar Associations Revealed by a Clustering Analysis of the Solar Neighborhood
DOI: 10.3847/1538-4357/ac8c25 Bibcode: 2022ApJ...939...94M

Faherty, Jacqueline K.; Gagné, Jonathan; Moranta, Leslie +1 more

We present the results of a density-based clustering analysis of the 6D XYZ Galactic positions and UVW-space velocities of nearby (≤200 pc) Gaia Early Data Release 3 stars with radial velocities using HDBSCAN, in opposition to previous studies (Kounkel & Covey 2019; Meingast et al. 2021) that only included positions and tangential velocities. …

2022 The Astrophysical Journal
Gaia 26
The mystery of unidentified infrared emission bands
DOI: 10.1007/s10509-022-04045-6 Bibcode: 2022Ap&SS.367...16K

Kwok, Sun

A family of unidentified infrared emission (UIE) bands has been observed throughout the Universe. The current observed spectral properties of the UIE bands are summarized. These properties are discussed in the frameworks of different models of the chemical carriers of these bands. The UIE carriers represent a large reservoir of carbon in the Unive…

2022 Astrophysics and Space Science
ISO 26
WO-type Wolf-Rayet Stars: The Last Hurrah of Massive Star Evolution
DOI: 10.3847/1538-4357/ac66e7 Bibcode: 2022ApJ...931..157A

Aadland, Erin; Massey, Philip; Hillier, D. John +3 more

Are WO-type Wolf-Rayet (WR) stars in the final stage of massive star evolution before core-collapse? Although WC- and WO-type WRs have very similar spectra, WOs show a much stronger O VI λλ3811,34 emission-line feature. This has usually been interpreted to mean that WOs are more oxygen rich than WCs, and thus further evolved. However, previous stu…

2022 The Astrophysical Journal
eHST 25
The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope
DOI: 10.3847/1538-3881/ac415b Bibcode: 2022AJ....163...61D

Gagliano, Robert; Kristiansen, Martti H.; LaCourse, Daryll M. +72 more

We report the discovery of TOI-2180 b, a 2.8 M J giant planet orbiting a slightly evolved G5 host star. This planet transited only once in Cycle 2 of the primary Transiting Exoplanet Survey Satellite (TESS) mission. Citizen scientists identified the 24 hr single-transit event shortly after the data were released, allowing a Doppler moni…

2022 The Astronomical Journal
Gaia 25
Constraining the Physical Properties of Stellar Coronal Mass Ejections with Coronal Dimming: Application to Far-ultraviolet Data of ϵ Eridani
DOI: 10.3847/1538-4357/ac80c1 Bibcode: 2022ApJ...936..170L

Loyd, R. O. Parke; France, Kevin; Youngblood, Allison +9 more

Coronal mass ejections (CMEs) are a prominent contributor to solar system space weather and might have impacted the Sun's early angular momentum evolution. A signal diagnostic of CMEs on the Sun is coronal dimming: a drop in coronal emission, tied to the mass of the CME, that is the direct result of removing emitting plasma from the corona. We pre…

2022 The Astrophysical Journal
SOHO eHST 25
A New Method for Direct Measurement of Isotopologue Ratios in Protoplanetary Disks: A Case Study of the 12CO/13CO Ratio in the TW Hya Disk
DOI: 10.3847/1538-4357/ac6efb Bibcode: 2022ApJ...932..126Y

Nomura, Hideko; Tsukagoshi, Takashi; Furuya, Kenji +2 more

Planetary systems are thought to be born in protoplanetary disks. Isotope ratios are a powerful tool for investigating the material origin and evolution from molecular clouds to planetary systems via protoplanetary disks. However, it is challenging to measure the isotope (isotopologue) ratios, especially in protoplanetary disks, because the emissi…

2022 The Astrophysical Journal
Gaia 25
The First Near-infrared Transmission Spectrum of HIP 41378 f, A Low-mass Temperate Jovian World in a Multiplanet System
DOI: 10.3847/2041-8213/ac559d Bibcode: 2022ApJ...927L...5A

Kirk, James; López-Morales, Mercedes; Alam, Munazza K. +22 more

We present a near-infrared transmission spectrum of the long-period (P = 542 days), temperate (T eq = 294 K) giant planet HIP 41378 f obtained with the Wide-Field Camera 3 instrument aboard the Hubble Space Telescope (HST). With a measured mass of 12 ± 3 M and a radius of 9.2 ± 0.1 R , HIP 41378 f has an extreme…

2022 The Astrophysical Journal
eHST 25
CME Evolution in the Structured Heliosphere and Effects at Earth and Mars During Solar Minimum
DOI: 10.1029/2022SW003215 Bibcode: 2022SpWea..2003215P

Nitta, Nariaki V.; Holmström, Mats; Futaana, Yoshifumi +13 more

The activity of the Sun alternates between a solar minimum and a solar maximum, the former corresponding to a period of "quieter" status of the heliosphere. During solar minimum, it is in principle more straightforward to follow eruptive events and solar wind structures from their birth at the Sun throughout their interplanetary journey. In this p…

2022 Space Weather
MEx SOHO 25
A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
DOI: 10.3847/1538-4357/ac3de5 Bibcode: 2022ApJ...926..155S

Kong, Xu; Zheng, Wei; Liu, Daizhong +10 more

We present ALMA 870 µm and JCMT/SCUBA2 850 µm dust continuum observations of a sample of optically dark and strongly lensed galaxies in cluster fields. The ALMA and SCUBA2 observations reach a median rms of ~0.11 mJy and 0.44 mJy, respectively, with the latter close to the confusion limit of the data at 850 µm. This represents on…

2022 The Astrophysical Journal
eHST 25
Detections of solar-like oscillations in dwarfs and subgiants with Kepler DR25 short-cadence data
DOI: 10.1051/0004-6361/202141168 Bibcode: 2022A&A...657A..31M

García, R. A.; Mosser, B.; Mathur, S. +6 more

During the survey phase of the Kepler mission, several thousand stars were observed in short cadence, allowing for the detection of solar-like oscillations in more than 500 main-sequence and subgiant stars. These detections showed the power of asteroseismology in determining fundamental stellar parameters. However, the Kepler Science Office discov…

2022 Astronomy and Astrophysics
Gaia 25