Protoplanetary disks of T Tauri binary systems in the Orion nebula cluster [PDF]
S. Daemgen +2 more
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The most powerful stellar flares driven by magnetic energy occur during the early pre-main-sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young stars, showing the greatest number of flares accessible to a single ...
Konstantin V. Getman +10 more
doaj +1 more source
Dynamics and Growth of Dust Grains in the Protoplanetary Nebula [PDF]
C. de la Fuente Marcos
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Individual and Average Behavior of Particles in a Protoplanetary Nebula [PDF]
P. Garaud +2 more
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A Comparison of Presolar Isotopic Signatures in Laboratory-Studied Primitive Solar System Materials and Comet 67P/Churyumov-Gerasimenko: New Insights from Light Elements, Halogens, and Noble Gases. [PDF]
Hoppe P, Rubin M, Altwegg K.
europepmc +1 more source
Paleomagnetic evidence for a disk substructure in the early solar system. [PDF]
Borlina CS +6 more
europepmc +1 more source
The (sub-)millimeter SED of protoplanetary disks in the outskirts of the Orion nebula cluster [PDF]
L. Ricci +7 more
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Carbon and oxygen isotope evidence for a protoplanetary disk origin of organic solids in meteorites. [PDF]
Lawrence WM, Blake GA, Eiler J.
europepmc +1 more source
Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]
Wang W +4 more
europepmc +1 more source
A SUBMILLIMETER ARRAY SURVEY OF PROTOPLANETARY DISKS IN THE ORION NEBULA CLUSTER [PDF]
Rita K. Mann, Jonathan P. Williams
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