Nebula
National Institutes of Health
Papers overview
Semantic Scholar uses AI to extract papers important to this topic.
We report the discovery of the new pulsar wind nebula (PWN) G141.2+5.0 in data observed with the Dominion Radio Astrophysical…
Based on axisymmetric hydrodynamical simulations and three-dimensional (3D) reconstructions with Shape, we investigate the…
We review our current understanding of the formation and early evolution of the solar nebula, the protoplanetary disk from which…
The growth of meter-sized bodies in the solar nebula by dust accretion is examined. The meter-sized bodies have velocity about 50…
The Luminous Blue Variable star η Carinae is one of the most massive stars known. It underwent a giant eruption in 1843 in which…
As dust aggregates settled toward the midplane of the solar nebula, a thin dust layer was formed. The rotational velocity was a…
The ISO spectrum of NGC 6302 is used, in conjunction with the visible and ultraviolet spectrum, to determine the nebular…
Based on HI maps covering the 3 600 square degrees area delimited by , we investigated the neutral hydrogen distribution in the…
Soft X-ray emission from the ring nebula NGC6888, formed by the stellar wind of the central WolfRayet star HD192163, has been…