Results 211 to 220 of about 22,722 (262)

Oceanic fronts shape hemispheric contrasts in polar stratospheric extremes. [PDF]

Nat Commun
Omrani NE, Ogawa F, Nakamura H, Lubis SW, Keenlyside NS, Paolini LF.   +5 more
europepmc   +1 more source

Exploring the sub-Neptune frontier with JWST. [PDF]

Proc Natl Acad Sci U S A
Madhusudhan N, Holmberg M, Constantinou S, Cooke GJ.   +3 more
europepmc   +1 more source

Pristine ices in a planet-forming disk revealed by heavy water. [PDF]

Nat Astron
Leemker M, Tobin JJ, Facchini S, Curone P, Booth AS, Furuya K, van 't Hoff MLR.   +6 more
europepmc   +1 more source

Climate Change and Cardiovascular Health: Advancing Resilient Action Beyond COP30. [PDF]

Glob Heart
Prabhakaran P, Berenstein C, Hamidi S, Vedanthan R, Münzel T.   +4 more
europepmc   +1 more source

The Effects of Temperature on the Growth, Survival, and Feeding of <i>Chrysaora pacifica</i> (Cnidaria: Scyphozoa) Ephyrae. [PDF]

Biology (Basel)
Shin KH, Choi KH.
europepmc   +1 more source

Core-envelope miscibility in sub-Neptunes and super-Earths. [PDF]

Nature
Gilmore T, Stixrude L.
europepmc   +1 more source

Improvement of merging processes in N-body simulations in circumstellar disks

Zimmermann M, Pilat-Lohinger E.
europepmc   +1 more source

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Formation and Evolution of Planets

Astrophysics and Space Science, 1994
The basic stages of the formation of the planets are considered. Decay of turbulence in the solar nebula allows the precipitation of dust particles to the solar nebula’s equatorial plane, their growth occurring by sticking at collisions and transformation into kilometer-sized bodies (planetesimals) partly by direct growth and partly via gravitational ...
V. S. Safronov, E. L. Ruskol
openaire   +1 more source

Formation of Stars and Planets

Astronomische Nachrichten, 2004
A01 Modeling the Resonant Planetary System GJ 876 A02 First Classification of Dusty Protoplanets A03 IDL-Models of Infrared Emission from Dust Objects (Applied to Dust in Comets) A04 Theoretical Predicitions and Observational Tests of the Migration Hypothesis A05 Towards Characterization of Exoplanetary Spectra with the VLT ...
Wuchterl, Günther, Guenther, Eike
openaire   +2 more sources

Extrasolar Planets: Constraints for Planet Formation Models

Science, 2005
Since 1995, more than 150 extrasolar planets have been discovered, most of them in orbits quite different from those of the giant planets in our own solar system. The number of discovered extrasolar planets demonstrates that planetary systems are common but also that they may possess a large variety of properties.
Nuno C, Santos, Willy, Benz, Michel, Mayor   +2 more
openaire   +2 more sources