Results 171 to 180 of about 239,171 (281)
We present high resolution adaptive optics (AO) corrected images of the silhouette disk Orion 218-354 taken with Magellan AO (MagAO) and its visible light camera, VisAO, in simultaneous differential imaging (SDI) mode at H-alpha.
Briguglio, Runa+13 more
core +1 more source
Expanding bubbles in Orion A: [C <sub>II</sub>] observations of M42, M43, and NGC 1977. [PDF]
Pabst CHM+9 more
europepmc +1 more source
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
Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows
The James Webb Space Telescope (JWST) observations have revolutionized extragalactic research, particularly with the discovery of little red dots (LRDs), which have been discovered as a population of dust-reddened broad-line active galactic nuclei (AGNs).
Zhengrong Li+4 more
doaj +1 more source
Chiroptical activity of gas-phase propylene oxide predicting the handedness of interstellar circular polarization in the presolar nebula. [PDF]
Garcia AD+5 more
europepmc +1 more source
Dust in the Orion Nebula [PDF]
N. C. Wickramasinghe, K. Nandy
openaire +2 more sources
A photometric survey of the stars of the Huygenian region of the Great Nebula of Orion [PDF]
Charles Newman Wunder
openalex +1 more source
Observations of the 145.5 micron (OI) emission line in the Orion nebula [PDF]
A first set of observations of the (OI) 3P to 3P1 (145.5 micron) transition was obtained. The line was observed both in a beam centered on the Trapezium, and in a 7 times wider beam encompassing most of the Orion Nebula. A wide beam map of the region was
Harwit, M.+3 more
core +1 more source