Results 161 to 170 of about 411,596 (264)
Doppler Tomography of the Circumstellar Disk of the Be Star κ Draconis
κ Draconis is a binary system with a classical Be star as the primary component. Its emission-line spectrum consists of hydrogen lines, notably the Hα line with peak intensity ratio (V/R) variations phase-locked with the orbital period P = 61.55 days ...
Ilfa A. Gabitova +4 more
doaj +1 more source
The V883 Ori system is a rapidly accreting young stellar object that has been used as a laboratory for studying the molecular inventory of young circumstellar disks with high luminosity.
Adolfo S. Carvalho +2 more
doaj +1 more source
We study the launching of magnetized jets from a resistive circumstellar disk within a binary system, employing a unique combination of 3D MHD jet launching simulations (PLUTO code) and post-processed 3D radiative transfer modeling (RADMC-3D code).
Somayeh Sheikhnezami +2 more
doaj +1 more source
SPITZERSPECTROSCOPY OF CIRCUMSTELLAR DISKS IN THE 5 Myr OLD UPPER SCORPIUS OB ASSOCIATION [PDF]
S. E. Dahm +3 more
openalex +1 more source
Exocomet Circumstellar Fe I Absorption in the Beta Pictoris Gas Disk [PDF]
Barry Y. Welsh, Sharon L. Montgomery
openalex +1 more source
Thermal Synthesis of Carbamic Acid and Its Dimer in Interstellar Ices: A Reservoir of Interstellar Amino Acids. [PDF]
Marks JH +6 more
europepmc +1 more source
Jets and outflows are commonly observed in young stellar objects, yet their origins remain debated. Using 3D nonideal magnetohydrodynamic (MHD) simulations of a circumstellar disk threaded by a large-scale open poloidal magnetic field, we identify three ...
Yisheng Tu +4 more
doaj +1 more source
Morphological components analysis for circumstellar disks imaging [PDF]
Benoît Pairet +2 more
openalex +1 more source
Improving signal-to-noise in the direct imaging of exoplanets and circumstellar disks with MLOCI [PDF]
Z. Wahhaj +12 more
openalex +1 more source
JWST MIRI MRS Observations of T Cha: Discovery of a Spatially Resolved Disk Wind
Understanding when and how circumstellar disks disperse is crucial to constrain planet formation and migration. Thermal winds powered by high-energy stellar photons have long been theorized to drive disk dispersal.
Naman S. Bajaj +10 more
doaj +1 more source

