Results 121 to 130 of about 172,889 (233)
Open questions on carbon-based molecules in space. [PDF]
Hansen CS +3 more
europepmc +1 more source
The Secular Evolution of Planetary Nebula IC 418 and Its Implications for Carbon Star Formation
The rate of stellar evolution can rarely be measured in real time. The fastest evolution (excluding event-driven evolution), where stars may evolve measurably over decades, is during the post–Asymptotic Giant Branch (AGB) phase. In this Letter we provide
Albert A. Zijlstra, Quentin A. Parker
doaj +1 more source
Gas phase synthesis of the C40 nano bowl C40H10. [PDF]
Tuli LB +8 more
europepmc +1 more source
Polarization properties of OH emission in planetary nebulae [PDF]
José F. Gómez +5 more
openalex +1 more source
I demonstrate the usage of planetary nebulae (PNe) to infer that a pair of jets shaped the ejecta of the core-collapse supernova (CCSN) SN 1987A. The main structure of the SN 1987A inner ejecta, the ‘keyhole’, comprises two low-intensity zones.
Noam Soker
doaj +1 more source
Shaping planetary nebulae with jets in inclined triple stellar systems [PDF]
Muhammad Akashi, Noam Soker
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Exploring the depths of Solar System evolution. [PDF]
Meyers SR, Peters SE.
europepmc +1 more source
Charge exchange of O3+ with H in planetary nebulae [PDF]
R. E. S. Clegg, J. R. Walsh
openalex +1 more source
Statistics — Spatial and Velocity Distribution of Planetary Nebulae [PDF]
J. H. Cahn, Stanley P. Wyatt
openalex +1 more source
Polycyclic aromatic hydrocarbons and molecular hydrogen in oxygen-rich planetary nebulae: the case of NGC 6720. [PDF]
Cox NL +4 more
europepmc +1 more source

