Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
The potential for planet formation of a circumstellar disk depends on the dust and gas reservoirs, which evolve as a function of the disk age. The Atacama Large Millimeter/submillimeter Array AGE-PRO Large Program has measured several disk properties ...
Nicolás T. Kurtovic +20 more
doaj +1 more source
Gas-phase synthesis of the bicyclic silicon tricarbide molecule (c-SiC<sub>3</sub>) as a precursor to silicon carbide nanoparticles in space. [PDF]
Goettl SJ +10 more
europepmc +1 more source
Crystallization of stardust analogs under an electron flux atmosphere. [PDF]
Shohan RA +6 more
europepmc +1 more source
Unconventional gas-phase preparation of the prototype polycyclic aromatic hydrocarbon naphthalene (C10H8) via the reaction of benzyl (C7H7) and propargyl (C3H3) radicals coupled with hydrogen-atom assisted isomerization. [PDF]
He C +9 more
europepmc +1 more source
The abundances of carbon and nitrogen in the atmospheres of classical Be stars. [PDF]
Peters GJ +4 more
europepmc +1 more source
Formation of free-floating planetary mass objects via circumstellar disk encounters. [PDF]
Fu Z, Deng H, Lin DNC, Mayer L.
europepmc +1 more source
Experimental evidence for granular shear-flow instability in the Epstein regime. [PDF]
Capelo HL +9 more
europepmc +1 more source
Circumstellar Gas-Disk Variability Around A-Type Stars: The Detection of Exocomets?
B. Welsh, Sharon L. Montgomery
semanticscholar +1 more source
Gas temperature distribution in the IRC + 10216 circumstellar envelope [PDF]
S. D. Doty, C. M. Leung
openaire +1 more source

