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The Open Cluster Chemical Abundances and Mapping Survey. VI. Galactic Chemical Gradient Analysis from APOGEE DR17
DOI: 10.3847/1538-3881/ac7ce5 Bibcode: 2022AJ....164...85M

Bizyaev, Dmitry; Cunha, Katia; Majewski, Steven R. +19 more

The goal of the Open Cluster Chemical Abundances and Mapping (OCCAM) survey is to constrain key Galactic dynamic and chemical evolution parameters by the construction and analysis of a large, comprehensive, uniform data set of infrared spectra for stars in hundreds of open clusters. This sixth contribution from the OCCAM survey presents analysis o…

2022 The Astronomical Journal
Gaia 39
TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
DOI: 10.3847/1538-3881/ac7cea Bibcode: 2022AJ....164...96C

Latham, David W.; Tamura, Motohide; Stassun, Keivan G. +53 more

Exploring the properties of exoplanets near or inside the radius valley provides insight on the transition from the rocky super-Earths to the larger, hydrogen-rich atmosphere mini-Neptunes. Here, we report the discovery of TOI-1452b, a transiting super-Earth (R p = 1.67 ± 0.07 R ) in an 11.1 day temperate orbit (T eq

2022 The Astronomical Journal
Gaia 38
Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-sized Exoplanet HD 106315c
DOI: 10.3847/1538-3881/ac85be Bibcode: 2022AJ....164..124K

Gorjian, Varoujan; Fortney, Jonathan J.; Mikal-Evans, Thomas +27 more

We present a transmission spectrum for the Neptune-sized exoplanet HD 106315c from optical to infrared wavelengths based on transit observations from the Hubble Space Telescope/Wide Field Camera 3, K2, and Spitzer. The spectrum shows tentative evidence for a water absorption feature in the 1.1-1.7 µm wavelength range with a small amplitude o…

2022 The Astronomical Journal
eHST 37
A Tendency Toward Alignment in Single-star Warm-Jupiter Systems
DOI: 10.3847/1538-3881/ac8153 Bibcode: 2022AJ....164..104R

Rice, Malena; Howard, Andrew W.; Dai, Fei +9 more

The distribution of spin-orbit angles for systems with wide-separation, tidally detached exoplanets offers a unique constraint on the prevalence of dynamically violent planetary evolution histories. Tidally detached planets provide a relatively unbiased view of the primordial stellar obliquity distribution, as they cannot tidally realign within th…

2022 The Astronomical Journal
Gaia 36
HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs
DOI: 10.3847/1538-3881/ac4a77 Bibcode: 2022AJ....163..125J

Hobson, M.; Jordán, Andrés; Palle, E. +35 more

The relative rarity of giant planets around low-mass stars compared with solar-type stars is a key prediction from the core-accretion planet formation theory. In this paper we report on the discovery of four gas giant planets that transit low-mass late K and early M dwarfs. The planets HATS-74Ab (TOI 737b), HATS-75b (TOI 552b), HATS-76b (TOI 555b)…

2022 The Astronomical Journal
Gaia 35
Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf
DOI: 10.3847/1538-3881/ac56e2 Bibcode: 2022AJ....163..189W

Fitzgerald, Michael P.; Skemer, Andrew; Wallack, Nicole L. +30 more

A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoretical evolutionary tracks, spectral synthesis, and atmospheric retrievals for substellar objects. Here, we report results of atmospheric retrieval on a synthetic spectrum …

2022 The Astronomical Journal
Gaia 34
A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions
DOI: 10.3847/1538-3881/ac517f Bibcode: 2022AJ....163..207C

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +111 more

Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 au) on the formation and evolution of exoplanets. We investigate these effects using new data from Gaia Early Data Release 3 and the Transiting Exoplanet Survey Satellite mission to characterize wide-binary systems with transiting e…

2022 The Astronomical Journal
Gaia 34
Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
DOI: 10.3847/1538-3881/ac4d9f Bibcode: 2022AJ....163..159R

Sing, David K.; Lothringer, Joshua D.; Reggiani, Henrique +2 more

Idealized protoplanetary disk and giant planet formation models have been interpreted to suggest that a giant planet's atmospheric abundances can be used to infer its formation location in its parent protoplanetary disk. It has recently been reported that the hot Jupiter WASP-77 A b has subsolar atmospheric carbon and oxygen abundances with a sola…

2022 The Astronomical Journal
Gaia 33
TOI-3714 b and TOI-3629 b: Two Gas Giants Transiting M Dwarfs Confirmed with the Habitable-zone Planet Finder and NEID
DOI: 10.3847/1538-3881/ac7804 Bibcode: 2022AJ....164...50C

Kobulnicky, Henry A.; Cochran, William D.; Mahadevan, Suvrath +36 more

We confirm the planetary nature of two gas giants discovered by the Transiting Exoplanet Survey Satellite to transit M dwarfs. TOI-3714 (V = 15.24, J = 11.74) is an M2 dwarf hosting a hot Jupiter (M p = 0.70 ± 0.03 M J and R p = 1.01 ± 0.03 R J ) on an orbital period of 2.154849 ± 0.000001 days wi…

2022 The Astronomical Journal
Gaia 33
The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109
DOI: 10.3847/1538-3881/ac479d Bibcode: 2022AJ....163..114E

Fang, Min; Edwards, Suzan; Banzatti, Andrea +59 more

The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program of low-mass pre-main-sequence stars, coupled with forthcoming data from Atacama Large Millimeter/submillimeter Array and James Webb Space Telescope, will provide the foundation to revolutionize our understanding of the relationship between…

2022 The Astronomical Journal
Gaia eHST 31