Results 81 to 90 of about 398,118 (263)
On the Planetary Interpretation of Multiple Gaps and Rings in Protoplanetary Disks Seen By ALMA [PDF]
It has been recently suggested that the multiple concentric rings and gaps discovered by ALMA in many protoplanetary disks may be produced by a single planet, as a result of the complex propagation and dissipation of the multiple spiral density waves it ...
Ryan Miranda, R. Rafikov
semanticscholar +1 more source
Abstract It has been proposed that IIE iron meteorites formed through impact processes on a parent body that was composed of either the H chondrites or a much‐debated fourth ordinary chondrite group, the HH chondrites. To resolve this debate, we have compiled a large dataset for the ordinary chondrites, low‐fayalite ungrouped chondrites, and IIE irons,
Rachel S. Kirby +2 more
wiley +1 more source
Substructures in Compact Disks of the Taurus Star-forming Region
Observations of substructure in protoplanetary disks have largely been limited to the brightest and largest disks, excluding the abundant population of compact disks, which are likely sites of planet formation.
Shangjia Zhang +7 more
doaj +1 more source
The origin of short-lived radionuclides and the astrophysical environment of solar system formation
Based on early solar system abundances of short-lived radionuclides (SRs), such as $^{26}$Al (T$_{1/2} = 0.74$ Myr) and $^{60}$Fe (T$_{1/2} = 1.5$ Myr), it is often asserted that the Sun was born in a large stellar cluster, where a massive star ...
Amelin Y. +15 more
core +1 more source
disksurf: Extracting the 3D Structure of Protoplanetary Disks [PDF]
Richard Teague +3 more
openalex +1 more source
ALMA survey of Class II protoplanetary disks in Corona Australis: a young region with low disk masses [PDF]
Context. In recent years, the disk populations in a number of young star-forming regions have been surveyed with the Atacama Large Millimeter/submillimeter Array (ALMA).
P. Cazzoletti +22 more
semanticscholar +1 more source
Close binary systems present challenges to planet formation. As binary separations decrease, so do the occurrence rates of protoplanetary disks in young systems and planets in mature systems.
Benjamin M. Tofflemire +10 more
doaj +1 more source
Dust in protoplanetary disks: observations*
Solid particles, usually referred to as dust, are a crucial component of interstellar matter and of planet forming disks surrounding young stars. Despite the relatively small mass fraction of ≈1% (in the solar neighborhood of our galaxy; this number may ...
Waters L.B.F.M.
doaj +1 more source
ALMA SURVEY OF LUPUS PROTOPLANETARY DISKS. I. DUST AND GAS MASSES [PDF]
We present the first high-resolution sub-millimeter survey of both dust and gas for a large population of protoplanetary disks. Characterizing fundamental properties of protoplanetary disks on a statistical level is critical to understanding how disks ...
M. Ansdell +14 more
semanticscholar +1 more source
Chemistry in Externally FUV-irradiated Disks in the Outskirts of the Orion Nebula Cluster
Most stars are born in stellar clusters, and their protoplanetary disks, which are the birthplaces of planets, can, therefore, be affected by the radiation of nearby massive stars.
Javiera K. Díaz-Berríos +6 more
doaj +1 more source

