Are presolar silicon carbide grains from novae actually from supernovae?

Nittler, L. R.; Hoppe, P.

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Are presolar silicon carbide grains from novae actually from supernovae?

Nittler, L. R., & Hoppe, P. (2005). Are presolar silicon carbide grains from novae actually from supernovae? Astrophysical Journal, 631(1), L89-L92.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-8A9C-A Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-8A9D-8

Genre: Journal Article

Alternative Title : Astrophys. J.

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Creators:
Nittler, L. R., Author
Hoppe, P.^{1, 2}, Author

Affiliations:
1Particle Chemistry, Max Planck Institute for Chemistry, Max Planck Society, ou_1826291
2Cosmochemistry, Max Planck Institute for Chemistry, Max Planck Society, ou_1826294

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Free keywords: dust, extinction; meteors, meteoroids; novae, cataclysmic variables; nuclear reactions, nucleosynthesis, abundances; supernovae : general

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Language(s): eng - English

Dates: Date issued: 2005-09-20

Publication Status: Issued

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Rev. Type: Peer

Identifiers: eDoc: 268054
ISI: 000231959400023

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Title: Astrophysical Journal

Alternative Title : Astrophys. J.

Source Genre: Journal

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Pages: - Volume / Issue: 631 (1) Sequence Number: - Start / End Page: L89 - L92 Identifier: ISSN: 0004-637X