Results 121 to 130 of about 4,999 (221)

Turbulent planetary nebulae around [WC]–type stars

open access: yes, 2002
Through a high-resolution spectroscopic survey, we analyze the velocity field of 16 planetary nebulae with [WC]- or wels-type nuclei in comparison with 8 nebulae having other central star types.
Y. Grosdidier   +3 more
core   +1 more source

Open questions on carbon-based molecules in space. [PDF]

open access: yesCommun Chem, 2022
Hansen CS   +3 more
europepmc   +1 more source

Gas phase synthesis of the C40 nano bowl C40H10. [PDF]

open access: yesNat Commun, 2023
Tuli LB   +8 more
europepmc   +1 more source

Spectroscopic Survey of Faint Planetary-nebula Nuclei. IV. The A35-type Central Star of Pa 27

open access: yesThe Astrophysical Journal
We present optical spectroscopy of the 12th-magnitude central star of the planetary nebula (PN) Patchick 27 (Pa 27), obtained during a survey of faint PN nuclei (PNNs) with the Low-Resolution Spectrograph of the Hobby–Eberly Telescope.
Howard E. Bond, Gregory R. Zeimann
doaj   +1 more source

A radio-continuum and photoionization-model study of the two planetary nebulae in the Sagittarius dwarf galaxy

open access: yes, 2000
Radio continuum observations at 1.4, 4.8 and 8.6 GHz of the two Planetary Nebulae (PNe) in the Sagittarius dwarf galaxy reveal the elongated shape ofWray 16-423 and the extreme compactness of He 2-436.
Dudziak, G.   +3 more
core  

Planetary Nebulae in the eROSITA eRASS1 Catalog

open access: yesThe Astrophysical Journal
Some planetary nebulae (PNs) host X-ray-emitting hot bubbles shaped by stellar wind interactions and/or harbor X-ray-emitting central stars due to accretion, shocks within their fast stellar winds, or even chromospheric emission from binary companions ...
Haoyang Yuan   +3 more
doaj   +1 more source

Exploring the depths of Solar System evolution. [PDF]

open access: yesProc Natl Acad Sci U S A, 2022
Meyers SR, Peters SE.
europepmc   +1 more source

Planetary nebulae

open access: yesScholarpedia, 2007
openaire   +1 more source

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