Results 21 to 30 of about 27,938 (255)

Complex molecules in the Orion Kleinmann-Low nebula

open access: yesBIO Web of Conferences, 2014
In the framework of the delivery to the early Earth of extraterrestrial molecules, we have studied complex molecular species toward the Orion Kleinmann-Low nebula. This nebula is rich in molecules as well as in nascent stars and planetary systems.
Despois D.   +7 more
doaj   +1 more source

On the distances of planetary nebulae. [PDF]

open access: yesThe Astronomical Journal, 1971
29 pages, 25 figures, 20 tables, 1 appendix. Submitted to MNRAS; revised to reference Frew et al.
openaire   +5 more sources

Integral Field Spectroscopy of Planetary Nebulae with MUSE

open access: yesGalaxies, 2020
The Multi-Unit Spectroscopic Explorer (MUSE) is a large integral field unit mounted on the ESO Very Large Telescope. Its spatial (60 arcsecond field) and wavelength (4800–9300Å) coverage is well suited to detailed imaging spectroscopy of extended ...
Jeremy R. Walsh, Ana Monreal-Ibero
doaj   +1 more source

The dynamics of Planetary Nebulae [PDF]

open access: yesSymposium - International Astronomical Union, 1997
In this review we focus on new observations and theory that directly pertain to understanding the hydrodynamic evolution of planetary nebulae (PNe). The recent history of the field lead us to break the review into two parts, macroscopic and microscopic structures, since both the size scales and the dominant physics appear to cleave nicely into more-or ...
Bruce Balick, Adam Frank
openaire   +2 more sources

Lessons from the Ionised and Molecular Mass of Post-CE PNe

open access: yesGalaxies, 2022
Close binary evolution is widely invoked to explain the formation of axisymmetric planetary nebulae after a brief common envelope phase. The evolution of the primary would be interrupted abruptly, its still quite massive envelope being fully ejected to ...
Miguel Santander-García   +4 more
doaj   +1 more source

On the Origin of Planetary Nebulae [PDF]

open access: yesProgress of Theoretical Physics, 1962
A hypothesis that planetary nebulae originate from red giants when tl:e helium burning begins in the degenerate helium core is proposed and examined quantitatively. It is assumed that the shock wave is generated by the rapid core expansion which is caused by the removal of degeneracy at the helium core.
Yasuo Tanaka, Shiro Sakashita
openaire   +2 more sources

Spectroscopy of Planetary Nebulae with Herschel: A Beginners Guide

open access: yesGalaxies, 2018
A brief overview of the Herschel Space Telescope PACS and SPIRE spectrographs is given, pointing out aspects of working with the data products that should be considered by anyone using them.
Katrina Exter
doaj   +1 more source

Irradiation Investigation: Exploring the Molecular Gas in NGC 7293

open access: yesGalaxies, 2020
Background: Many planetary nebulae retain significant quantities of molecular gas and dust despite their signature hostile radiation environments and energetic shocks.
Jesse Bublitz   +7 more
doaj   +1 more source

Molecules in planetary nebulae [PDF]

open access: yesThe Astrophysical Journal, 1978
The study of molecules in planetary nebulae is still in its infancy; therefore, it is appropriate both to review existing knowledge and to anticipate developments that will arise as the subject matures. Briefly stated, this subject consists of observations of hydrogen, H2, and carbon monoxide, CO, molecules in a very few nebulae; the tentative ...
openaire   +2 more sources

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