Results 91 to 100 of about 48,210 (191)
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
Evidence for a Binary origin of the Young Planetary Nebula HB 12 [PDF]
Young planetary nebulae play an important role in stellar evolution when intermediate- to low-mass stars (0.8 ~ 8 M) evolve from the proto-planetary nebulae phase to the planetary nebulae phase. Many young planetary nebulae display distinct bipolar structures as they evolve away from the proto-planetary nebulae phase.
arxiv
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
doaj +1 more source
Earth's volatile depletion trend is consistent with a high-energy Moon-forming impact. [PDF]
Solomatova NV, Caracas R.
europepmc +1 more source
Internal Motions in the Planetary Nebula IC 4997 [PDF]
O. C. Wilson, C. R. O’dell
openalex +1 more source
New Close Binary Central Stars of Planetary Nebulae from Gaia DR3 Epoch Photometry. [PDF]
Chornay N, Walton NA.
europepmc +1 more source
On the Variability of the Central Star of the Planetary Nebula HZ 1–5 [PDF]
G. H. Herbig, A. A. Boyarchuk
openalex +1 more source