Results 21 to 30 of about 3,157,542 (333)

Dense gas in a giant molecular filament [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context. Recent surveys of the Galactic plane in the dust continuum and CO emission lines reveal that large (≳50 pc) and massive (≳105 M⊙) filaments, know as giant molecular filaments (GMFs), may be linked to Galactic dynamics and trace the mid-plane of the gravitational potential in the Milky Way.
Y. Wang   +12 more
openaire   +5 more sources

Retention of Long-period Gas Giant Planets: Type II Migration Revisited [PDF]

open access: yes, 2020
During their formation, emerging protoplanets tidally interact with their natal disks. Proto-gas-giant planets, with Hills radius larger than the disk thickness, open gaps and quench gas flow in the vicinity of their orbits.
Yi-Xian Chen   +4 more
semanticscholar   +1 more source

Forming Gas Giants around a Range of Protostellar M-dwarfs by Gas Disk Gravitational Instability

open access: yesThe Astrophysical Journal, 2023
Recent discoveries of gas giant exoplanets around M-dwarfs from transiting and radial velocity surveys are difficult to explain with core-accretion models. We present here a homogeneous suite of 162 models of gravitationally unstable gaseous disks. These
Alan P. Boss, Shubham Kanodia
doaj   +1 more source

Breaking Degeneracies in Formation Histories by Measuring Refractory Content in Gas Giants

open access: yesThe Astrophysical Journal, 2023
Relating planet formation to atmospheric composition has been a long-standing goal of the planetary science community. So far, most modeling studies have focused on predicting the enrichment of heavy elements and the C/O ratio in giant planet atmospheres.
Yayaati Chachan   +3 more
doaj   +1 more source

Investigating Trends in Atmospheric Compositions of Cool Gas Giant Planets Using Spitzer Secondary Eclipses [PDF]

open access: yesAstronomical Journal, 2019
We present new 3.6 and 4.5 μm secondary eclipse measurements for five cool (T ≲ 1000 K) transiting gas giant planets: HAT-P-15b, HAT-P-17b, HAT-P-18b, HAT-P-26b, and WASP-69b.
N. Wallack   +9 more
semanticscholar   +1 more source

Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810 [PDF]

open access: yesAstronomical Journal, 2018
The N2K planet search program was designed to exploit the planet-metallicity correlation by searching for gas giant planets orbiting metal-rich stars. Here, we present the radial velocity measurements for 378 N2K target stars that were observed with the ...
K. Ment   +4 more
semanticscholar   +1 more source

MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star [PDF]

open access: yesAstronomical Journal, 2019
We report the discovery of a gas-giant planet orbiting a low-mass host star in the microlensing event MOA-bin-29 that occurred in 2006. We find five degenerate solutions with the planet/host-star mass ratio of q ∼ 10−2.
I. Kondo   +34 more
semanticscholar   +1 more source

Long-term Stability of Planetary Systems Formed from a Transitional Disk

open access: yesThe Astrophysical Journal, 2023
Transitional disks are protoplanetary disks with large and deep central holes in the gas, possibly carved by young planets. Dong & Dawson simulated systems with multiple giant planets that were capable of carving and maintaining such gaps during the disk
Rory Bowens   +3 more
doaj   +1 more source

Tidally Heated Exomoons around Gas Giants [PDF]

open access: yesThe Planetary Science Journal, 2021
Abstract Thousands of exoplanets have been discovered; however, the detection of exomoons remains elusive. Tidally heated exomoons have been proposed as candidate targets for observation; vigorous tidal dissipation can raise the moon’s surface temperature, making direct imaging possible, and cause widespread volcanism that can have a ...
Marc Rovira-Navarro   +3 more
openaire   +4 more sources

H− Opacity and Water Dissociation in the Dayside Atmosphere of the Very Hot Gas Giant WASP-18b [PDF]

open access: yes, 2018
We present one of the most precise emission spectra of an exoplanet observed so far. We combine five secondary eclipses of the hot Jupiter WASP-18b (Tday ∼ 2900 K) that we secured between 1.1 and 1.7 μm with the Wide Field Camera 3 instrument on board ...
J. Arcangeli   +9 more
semanticscholar   +1 more source

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