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About this Physics and Astronomy article

Predicting the fate of binary red giants using the observed sequence E star population: binary planetary nebula nuclei and post-RGB stars by J. D. Nie; P. R. Wood; C. P. Nicholls is a Physics and Astronomy article available to read on EtoBox.

It is typically read by researchers, students, and practitioners in Physics and Astronomy.

Author
J. D. Nie; P. R. Wood; C. P. Nicholls
Publisher
John Wiley and Sons; Oxford University Press; Oxford University Press (OUP) (ISSN 0035-8711)
Published
2012
Language
EN
Field
Physics and Astronomy (Physical Sciences)

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