Hot, fast planetary nebula haloes: a natural consequence of clumpy cores

Arthur, S. J.; Dyson, J. E.; Hartquist, T. W.

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Hot, fast planetary nebula haloes: a natural consequence of clumpy cores

Arthur, S. J., Dyson, J. E., & Hartquist, T. W. (1994). Hot, fast planetary nebula haloes: a natural consequence of clumpy cores. Revista Mexicana de Astronomia y Astrofisica, 29, 84-87.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-EF18-8 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-EF19-6

Genre: Journal Article

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Creators:
Arthur, S. J., Author
Dyson, J. E., Author
Hartquist, T. W.¹, Author

Affiliations:
1Theory and Complex Plasmas, MPI for Extraterrestrial Physics, Max Planck Society, ou_159894

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Language(s): eng - English

Dates: Date issued: 1994

Publication Status: Issued

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Rev. Type: Internal

Identifiers: eDoc: 237893

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Title: Revista Mexicana de Astronomia y Astrofisica

Alternative Title : Rev. Mex. Astron. Astrofis.

Source Genre: Journal

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Pages: - Volume / Issue: 29 Sequence Number: - Start / End Page: 84 - 87 Identifier: ISSN: 0185-1101