AKARI/IRC observations of heavily obscured oxygen-rich AGB and post-AGB stars
We present AKARI/IRC observations of a sample of six extremely red IRAS sources, of which three are variable OH/IR stars and the rest are early post-AGB stars. The OH/IR stars show a red continuum with the expected strong 10 micron silicate absorption feature, while the post-AGB stars show an even redder continuum accompanied with a comparably weak ...
Bunzel, F. +4 more
openaire +2 more sources
Nitrogen Addition Affects Ecosystem Carbon Exchange by Regulating Plant Community Assembly and Altering Soil Properties in an Alpine Meadow on the Qinghai-Tibetan Plateau. [PDF]
Han L +9 more
europepmc +1 more source
Interferometric studies of AGB and post-AGB stars
Several classes of evolved stars contain highly luminous objects, which, more often than not, are characterized by strong mass loss. Two fundamental properties that lie at the basis of their outer appearance and internal evolution, as well as that of the galaxies in which they are embedded.
openaire +1 more source
Investigation of potential safety hazards during medical waste disposal in SARS-CoV-2 testing laboratory. [PDF]
Lv J, Yang J, Xue J, Zhu P, Liu L, Li S.
europepmc +1 more source
The abundance of S- and Si-bearing molecules in O-rich circumstellar envelopes of AGB stars. [PDF]
Massalkhi S +3 more
europepmc +1 more source
An evolutionary system of mineralogy. Part I: Stellar mineralogy (>13 to 4.6 Ga). [PDF]
Hazen RM, Morrison SM.
europepmc +1 more source
The mystery of unidentified infrared emission bands. [PDF]
Kwok S.
europepmc +1 more source
Chemical equilibrium in AGB atmospheres: Successes, failures, and prospects for small molecules, clusters, and condensates. [PDF]
Agúndez M +4 more
europepmc +1 more source
Phosphorus-rich stars with unusual abundances are challenging theoretical predictions. [PDF]
Masseron T +6 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

