Results 81 to 90 of about 2,529 (169)

The K2 and TESS Synergy. III. Search and Rescue of the Lost Ephemeris for K2's First Planet

open access: yesThe Astronomical Journal
K2-2 b/HIP 116454 b, the first exoplanet discovery by K2 during its Two-Wheeled Concept Engineering Test, is a sub-Neptune (2.5 ± 0.1 R _⊕ , 9.7 ± 1.2 M _⊕ ) orbiting a relatively bright ( K _S = 8.03) K-dwarf star on a 9.1 day period. Unfortunately, due
Erica Thygesen   +15 more
doaj   +1 more source

White Dwarf Stars in the Big Data Era

open access: yesAstronomische Nachrichten, Volume 346, Issue 1, January 2025.
ABSTRACT White dwarf stars are the most common endpoint of stellar evolution. Therefore, these old, numerous and compact objects provide valuable information on the late stages of stellar evolution, the physics of dense plasma and the structure and evolution of our Galaxy.
Maria Camisassa
wiley   +1 more source

From Underground Oceans to Continents: A Glimpse into the Water Inventory on Rocky Planets Using Host Star Abundances

open access: yesThe Astrophysical Journal
The amount of surface water is thought to be critical for a planet’s climate stability and thus habitability. However, the probability that a rocky planet may exhibit surface water at any point in its evolution is dependent on multiple factors, such as ...
Kiersten M. Boley   +4 more
doaj   +1 more source

Architectures of Planetary Systems. II. Trends with Host Star Mass and Metallicity

open access: yesThe Astronomical Journal
The current census of planetary systems displays a wide range of architectures. Extending earlier work, this paper investigates the correlation between our classification framework for these architectures and host stellar properties.
Alex R. Howe   +2 more
doaj   +1 more source

Effect of Uncertainty in Water Vapor Continuum Absorption on CO2 Forcing, Longwave Feedback, and Climate Sensitivity

open access: yesJournal of Advances in Modeling Earth Systems, Volume 16, Issue 7, July 2024.
Abstract We investigate the effect of uncertainty in water vapor continuum absorption at terrestrial wavenumbers on CO2 forcing F $\mathcal{F}$, longwave feedback λ, and climate sensitivity S $\mathcal{S}$ at surface temperatures Ts between 270 and 330 K.
Florian E. Roemer   +3 more
wiley   +1 more source

Where Are the Water Worlds? Identifying Exo-water-worlds Using Models of Planet Formation and Atmospheric Evolution

open access: yesThe Astrophysical Journal
Planet formation models suggest that the small exoplanets that migrate from beyond the snowline of the protoplanetary disk likely contain water-ice-rich cores (∼50% by mass), also known as water worlds.
Aritra Chakrabarty, Gijs D. Mulders
doaj   +1 more source

Lessons from the apparent peculiar nature of the star TYC 6544‐3483‐1

open access: yesAstronomische Nachrichten, Volume 345, Issue 4, May 2024.
Abstract We report a radio and optical study of the star TYC 6544‐3483‐1 originally selected as a follow‐up target in the course of our efforts to cross‐identify Galactic high‐energy sources. The star by itself finally turned out to be a very ordinary main‐sequence star despite the initial expectations that apparently pointed to the contrary.
Josep Martí   +5 more
wiley   +1 more source

Planet Masses, Radii, and Orbits from NASA’s K2 Mission

open access: yesThe Astrophysical Journal Supplement Series
We report the masses, sizes, and orbital properties of 86 planets orbiting 55 stars observed by NASA’s K2 Mission with follow-up Doppler measurements by the HIRES spectrometer at the W. M.
Andrew W. Howard   +52 more
doaj   +1 more source

Exo-MerCat v2.0.0: Updates and open-source release of the Exoplanet Merged Catalog software

open access: yesAstronomy and Computing
18 pages, 3 figures. Accepted for publication on Astronomy and Computing.
Eleonora Alei   +10 more
openaire   +3 more sources

HST astrometry of the closest brown dwarfs‐II. Improved parameters and constraints on a third body

open access: yesAstronomische Nachrichten, Volume 345, Issue 1, January 2024.
Abstract Located at less than two pc away, Luhman 16 AB (WISE J104915.57‐531906.1) is the closest pair of brown dwarfs and the third closest “stellar” system to Earth. An exoplanet candidate in the Luhman 16 binary system was reported in 2017 based on a weak astrometric signature in the analysis of 12 HST epochs.
L. R. Bedin   +7 more
wiley   +1 more source

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