Results 21 to 30 of about 586 (186)
Detection of DCO+in a circumstellar disk [PDF]
Accepted by A&A Letters; 4 pages, 1 ...
Dishoeck, E.F. +2 more
openaire +5 more sources
Processed and Unprocessed Ices in Circumstellar Disks [PDF]
AbstractWe present 3-5 µm VLT-ISAAC spectroscopy showing the presence of methanol ices in edge-on disks of young embedded stars. Examples include the disks of L1489 IRS in Taurus and CRBR 2422.8-3423 in Ophiuchus, the last of which has the highest column density of solid CO known toward a YSO.
Pontoppidan, K. +3 more
openaire +2 more sources
Spectropolarimetry and the Study of Circumstellar Disks [PDF]
Circumstellar disks play an important role in many stages of the evolution of stars. However, it is only possible to directly image circumstellar disks for a few of the nearest stars. For massive stars, the situation is even more difficult, as they are on average further away than the more numerous low mass stars.
openaire +2 more sources
Unveiling the Circumstellar Envelope and Disk: A Subarcsecond Survey of Circumstellar Structures [PDF]
47 Pages, 18 Figures, ApJ ...
Looney, Leslie W. +2 more
openaire +2 more sources
We report Atacama Large Millimeter/submillimeter Array (ALMA) polarization observations at 3 and 0.9 mm toward the GG Tau A system. In the ring, the percentage is relatively homogeneous at 3 mm, being 1.2%, while it exhibits a clear radial variation at 0.
Ya-Wen Tang +9 more
doaj +1 more source
Planet–planet scattering in circumstellar gas disks [PDF]
Astronomy and Astrophysics Letters, in ...
MARZARI, FRANCESCO +2 more
openaire +2 more sources
Microlensing of Circumstellar Disks
9 pages, 7 figures.
Zheng, Zheng, Ménard, Brice
openaire +2 more sources
Young protostellar binary systems, with expected ages less than ∼10 ^5 yr, are little modified since birth, providing key clues to binary formation and evolution. We present a first look at the young, Class 0 binary protostellar system R CrA IRAS 32 from
Frankie J. Encalada +21 more
doaj +1 more source
Long-term optical variability of high-mass X-ray binaries
Context. Systems known as Be/X-ray binaries form the most numerous group of high-mass X-ray binaries. Their long-term optical and infrared variability reflects the evolution of the circumstellar disk around the luminous companion.
Reig P., Blinov D., Tzouvanou A.
doaj +1 more source
Confined Chemistry in Space: Zeolite‐Supported Fe13 Nanoclusters Modulate CS Reactivity
The study explores how an Fe13 cluster confined in chabazite reshapes the reaction of CS and H2 under astrochemical conditions. Confinement promotes C–S bond cleavage over hydrogenation, directing chemistry toward CH4 and H2S formation. Additional CS enables CS2 and C2 species. Microkinetic analysis identifies protoplanetary environments where zeolites
Gerard Pareras, Albert Rimola
wiley +1 more source

