Results 171 to 180 of about 5,220,245 (377)
High Resolution ALMA Data of the Fomalhaut Debris Disk Confirms Apsidal Width Variation
We present long-baseline observations of the Fomalhaut outer debris disk at 223 GHz (1.3 mm) from Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 5, which we use along with archival short-baseline observations to produce a 0 $\mathop{.}\limits{^
Jay S. Chittidi +13 more
doaj +1 more source
Collisional properties of cm-sized high-porosity ice and dust aggregates and their applications to early planet formation [PDF]
Rainer Schräpler +2 more
openalex +1 more source
28 pages, 4 figures, for Journal of Cosmology proceedings of the Lorentz Center Workshop on New Directions in Modern Cosmology, Leiden NL Sept. 27-Oct.
Schild, Rudolph E., Gibson, Carl H.
openaire +2 more sources
High‐entropy perovskite nanofibers serve as robust and active bifunctional air electrodes in reversible protonic ceramic electrochemical cells. Their compositional complexity stabilizes the lattice, enriches oxygen vacancies, and accelerates surface exchange.
Hyeonggeun Kim +4 more
wiley +1 more source
exoALMA. XV. Interpreting the Height of CO Emission Layer
The availability of exquisite data and the development of new analysis techniques have enabled the study of emitting heights in protoplanetary disks. In this paper, we introduce a simple model linking the emitting height of CO to the disk surface density
Giovanni P. Rosotti +34 more
doaj +1 more source
Formation, Dynamical Evolution, and Habitability of Planets in Binary Star Systems [PDF]
Nader Haghighipour
openalex +1 more source
AB Aurigae: possible evidence of planet formation through the gravitational instability [PDF]
James Cadman, Ken Rice, Cassandra Hall
openalex +1 more source
Multiple Twinning in Nacre and Aragonite
Electron backscatter diffraction map of a cluster of geologic aragonite, exhibiting single, double, and triple twins. The whole cluster is approximately 2 cm wide. Colors indicate crystal orientations, so that pixels where the a‐, b‐, and c‐axis is perpendicular to the image plane are green, red, and blue, respectively.
Connor A. Schmidt +7 more
wiley +1 more source
A Neural Network Subgrid Model of the Early Stages of Planet Formation [PDF]
Thomas Pfeil +5 more
openalex +1 more source

