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  On the Transition Rate of the Fe x Red Coronal Line

Brenner, G., Crespo López-Urrutia, J. R., Bernitt, S., Fischer, D., Ginzel, R., Kubicek, K., et al. (2009). On the Transition Rate of the Fe x Red Coronal Line. Astrophysical Journal, 703(1), 68-73. doi:10.1088/0004-637X/703/1/68.

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 Creators:
Brenner, G.1, Author           
Crespo López-Urrutia, J. R.1, Author           
Bernitt, S.1, Author           
Fischer, D.2, Author           
Ginzel, R.1, Author           
Kubicek, K.1, Author           
Mäckel, V.1, Author           
Mokler, P. H.1, Author           
Simon, M. C.1, Author           
Ullrich, J.1, Author           
Affiliations:
1Division Prof. Dr. Joachim H. Ullrich, MPI for Nuclear Physics, Max Planck Society, ou_904547              
2Daniel Fischer - Emmy Noether Junior Research Group, Junior Research Groups, MPI for Nuclear Physics, Max Planck Society, ou_907553              

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Free keywords: atomic data; atomic processes; line: profiles; plasmas; stars: coronae; Sun: corona
 Abstract: We present a lifetime measurement of the 3s 23p 5 2 Po 1/2 first excited fine-structure level of the ground state configuration in chlorine-like Fe X, which relaxes to the ground state through a magnetic dipole (M1) transition (the so-called red coronal line) with a wavelength accurately determined to 637.454(1) nm. Moreover, the Zeeman splitting of line was observed. The lifetime of 14.2(2) ms is the most precise one measured in the red wavelength region and agrees well with advanced theoretical predictions and an empirically scaled interpolation based on experimental values from the same isoelectronic sequence.

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Language(s): eng - English
 Dates: 2009-08-25
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 441474
DOI: 10.1088/0004-637X/703/1/68
 Degree: -

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Title: Astrophysical Journal
  Alternative Title : ApJ
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 703 (1) Sequence Number: - Start / End Page: 68 - 73 Identifier: -