Results 141 to 150 of about 10,374 (277)
Abstract β Pictoris's well-studied debris disk and two known giant planets, in combination with the stability of the Hubble Space Telescope’s Space Telescope Imaging Spectrograph (HST/STIS) (and now also JWST), offers a unique opportunity to test planet–disk interaction models and to observe recent planetesimal ...
Arin M. Avsar +4 more
openaire +3 more sources
Direct Measurement of Explosive Impulse From Contact to the Ultra‐Near Field
ABSTRACT Measurement of impulse from explosive charges in contact and ultra‐near‐field regimes remains poorly characterised due to the short duration of loading, high strain rates, and the difficulty of obtaining direct momentum‐based measurements.
R. Alford +3 more
wiley +1 more source
Breaking Giant Chains: Early-stage Instabilities in Long-period Giant Planet Systems
Orbital evolution is a critical process that sculpts planetary systems, particularly during their early stages where planet–disk interactions are expected to lead to the formation of resonant chains.
Vighnesh Nagpal +2 more
doaj +1 more source
The relationship between equatorial wave interaction and heavy rainfall in Southeast Asia
This study examines the statistical relationship between co‐occurring equatorial waves and heavy rainfall in Southeast Asia. Heavy rainfall is more closely related to combined wave activity than to individual waves in many regions of Southeast Asia. The figure shows GPM–IMERG rainfall (shading) and ERA5 850‐hPa winds (vectors) composited on days when ...
Samantha Ferrett +7 more
wiley +1 more source
The Earliest Stage of Planet Formation: Numerical Simulations of Disk-planet Interaction and Observations of Protoplanetary Disks [PDF]
Planets form in protoplanetary disks. In disks, planets excite structures such as spiral density waves, and may clear material around their orbits to form gaps, through gravitational disk-planet interactions. By identifying these structures and comparing
Dong, Ruobing
core
While stellar jets and outflows are fueled by accretion from disks, their direct influence on disks remain unexplored. Here, we revisit Atacama Large Millimeter/submillimeter Array observations of ^12 CO ( J = 2–1) line emission for the young stellar ...
Masataka Aizawa +2 more
doaj +1 more source
Context. The multitude of different architectures found for evolved exoplanet systems are in all likelihood set during the initial planet-formation phase in the circumstellar disk. To understand this process, we have to study the earliest phases of planet formation. Aims.
C. Ginski +30 more
openaire +5 more sources
ABSTRACT Grass mowing is one of the most resource‐consuming activities in green maintenance, whether in private areas such as home gardens or in public spaces like urban parks. In recent years, concerns related to climate change, human health, and sustainability have become increasingly prominent in green maintenance, leading manufacturers and industry
Andrea Palladini +3 more
wiley +1 more source
Preprocessing Procedure for Propagation Measurements on MEO Satellite Links
ABSTRACT This paper presents a software tool designed for preprocessing data from an experimental campaign aimed at characterizing the tropospheric propagation channel using Medium Earth Orbit (MEO) satellites. The collected data provide critical insights into the channel in scenarios involving continuous variations in azimuth and elevation, along with
Marlene Brás +2 more
wiley +1 more source
Planetary system evolution: Planet-disk interactions and planet ejection from binary systems [PDF]
Throughout the evolution of a planetary system, planets, especially those newly formed, interact by several means with a variety of the system's constituents. In particular, the influence of the most massive planets is expected to govern much of the long-
Mudryk, Lawrence Russell
core +1 more source

