Results 101 to 110 of about 174,483 (232)
Detection of CH in the O-rich Planetary Nebula NGC 6302
Planetary nebulae are sites where ejected stellar material evolves into complex molecules, but the precise physical conditions and chemical routes that govern these processes are unclear.
Charmi Bhatt +35 more
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Spectroscopic observations of various tracers in nearby galaxies, such as Andromeda (M31), play a crucial role in identifying and classifying individual stellar populations and nebular objects, thereby enhancing our understanding of galactic composition,
Pinjian Chen +7 more
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We present a brief review of the formation and evolution of hydrogen-deficient central stars of planetary nebulae. We include a detailed description of the main observable features of both the central stars and their surrounding nebulae and review their ...
Marcelo M. Miller Bertolami
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Chemical abundances in Galactic planetary nebulae from faint emission lines [PDF]
J. García–Rojas
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MILAN Sky Survey, a dataset of raw deep sky images captured during one year with a Stellina automated telescope. [PDF]
Parisot O +5 more
europepmc +1 more source
Expansion Velocities of [NII] and [OIII] from Compact Planetary Nebulae [PDF]
Katsunori M. Shibata, Shinichi Tamura
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Polarization properties of OH emission in planetary nebulae [PDF]
José F. Gómez +5 more
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Statistics — Spatial and Velocity Distribution of Planetary Nebulae [PDF]
J. H. Cahn, Stanley P. Wyatt
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The physics of recombination lines in the He i singlet system is expected to be relatively simple, supported by accurate atomic models. We examine the intensities of He i singlets λ 3614, λ 3965, λ 5016, λ 6678, and λ 7281 and the triplet He i λ 5876
J. E. Méndez-Delgado +13 more
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