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  Probable detection of a bright infrared coronal emission line of SI IX near 3.93 microns

Kuhn, J. R., MacQueen, R. M., Streete, J., Tansey, G., Mann, I., Hillebrand, P., et al. (1999). Probable detection of a bright infrared coronal emission line of SI IX near 3.93 microns. Astrophysical Journal, 521, 478-482.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-E1B6-B Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-E1B7-9
Genre: Journal Article

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 Creators:
Kuhn, J. R., Author
MacQueen, R. M., Author
Streete, J., Author
Tansey, G., Author
Mann, I.1, Author              
Hillebrand, P., Author
Coulter, R., Author
Lin, H., Author
Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 Dates: 1999
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: BibTex Citekey: Kuhn:1999-418
 Degree: -

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Title: Astrophysical Journal
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 521 Sequence Number: - Start / End Page: 478 - 482 Identifier: -