Results 141 to 150 of about 27,938 (255)
A Dust-Scattering Model for M1-92: A Revised Estimate of the Mass Distribution and Inclination
Preplanetary nebulae (PPNe) are formed from mass-ejecting late-stage AGB stars. Much of the light from the star gets scattered or absorbed by dust particles, giving rise to the observed reflection nebula seen at visible and near-IR wavelengths ...
Yun Qi Li+2 more
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Internal Motions in the Planetary Nebula IC 4997 [PDF]
O. C. Wilson, C. R. O’dell
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We report our discovery of a faint nebula surrounding a previously little-studied 15th mag variable star, ASASSN-19ds, in the Southern Hemisphere constellation Antlia. Spectra verify that the star is a cataclysmic variable (CV).
Howard E. Bond+4 more
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On the Variability of the Central Star of the Planetary Nebula HZ 1–5 [PDF]
G. H. Herbig, A. A. Boyarchuk
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Oldhamite: a new link in upper mantle for C-O-S-Ca cycles and an indicator for planetary habitability. [PDF]
Liu Y+9 more
europepmc +1 more source
Dynamical Evolution of a Model Planetary Nebula [PDF]
William G. Mathews
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Earth's volatile depletion trend is consistent with a high-energy Moon-forming impact. [PDF]
Solomatova NV, Caracas R.
europepmc +1 more source
Echelle Studies on the Symmetrical Stratified Planetary Nebula NGC 3918 [PDF]
M. A. Dopita
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Optical Spectroscopy and Photoionization Model of Planetary Nebula NGC 6572
We investigated NGC 6572 through optical spectroscopy to determine its kinematical and chemical properties. Two intermediate dispersion spectra (R~5000) centered around Hα and Hβ were used to derive the nebular expansion velocity from emission lines ...
Muhammad Fajrin+2 more
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