Dutrey, A., 1999. Latest stages of star formation and circumstellar environment of young stellar objects. In: Mariotti, J.M., Alloin, D. (Eds.), Planets Outside the Solar System: Theory and Observation. Kluwer, Dortrecht, pp. 13-49....
These detections establish that benzonitrile is not unique to TMC-1; rather, aromatic chemistry appears to be widespread throughout the earliest stages of star formation, probably persisting at least until the initial formation of a protostar. The abundance of benzonitrile far exceeds predictions from...
lending the dance a sense of deep cultural significance," Zheng said. "Holding a cloth snake, the lead dancer mimics the snake's fluid movements, weaving his way through the dance troupe. His graceful steps and gestures guide the team's direction, rhythm and formation, making...
Each of the three cores is slightly different in mass, temperature, gas motions, and substructure, perhaps in part because they are in different stages in their star formation activity. The astronomers find magnetic fields in all three of the clumps, but the strengths also differ slightly from ...
“So, in short, the outcome of planet formation depends on the evolution and dispersal of the disk,” Bajaj said. At the heart of this discovery is the observation of T Cha, a young star – relative to the sun, which is about 4.6 billion years old – enveloped by an eroding circumste...
We propose a dedicated, ultra-deep spectroscopic survey in the near infrared (NIR), that will target a mass-limited sample of galaxies during two of the mo
We present a first study of the star-forming compact dust condensations revealed by <italic>Herschel</italic> in the two 2° × 2° Galactic Plane fields centered at [<inline-formula content-type="tex"/>, <italic>b</italic>] = [30°, 0°] and [<inline-f
stars: formationstars: pre-main sequenceWe present a first study of the star-forming compact dust condensations revealed by Herschel in the two 2 imes 2 \\degr Galactic Plane fields centered at [l;b] = [30\\degr; 0 \\degr] and [l;b] = [59\\degr; 0 \\degr], respectively, and...
Deep Insights into the Processes Occurring during Early Stages of the Formation and Room-Temperature Evolution of the Core (Amorphous SiO2)@Shell (Organo... Bosnar,Sanja,Jelic,... - 《Journal of Physical Chemistry C Nanomaterials & Interfaces》 被引量: 0发表: 2018年 Deep Insights into the Pro...
Although these approaches are sensitive to the formation of fibrillar structures, they reveal less about earlier aggregation stages, namely nucleation and oligomerization, which can themselves be very complex. Single-molecule (SM) methods are particularly well-suited to studying these early stages45,46,...