Issue |
Astron. Astrophys. Suppl. Ser.
Volume 129, Number 3, May I 1998
|
|
---|---|---|
Page(s) | 435 - 443 | |
DOI | https://doi.org/10.1051/aas:1998196 | |
Published online | 15 May 1998 |
Identification of FeH molecular lines in the spectrum of a sunspot umbra
1
Astronomy Department, Faculty of Science, Cairo University, Cairo, Egypt
2
currently: Institut für Theoretische Astrophysik der Universität Heidelberg, Tiergartenstrasse 15, D-69121 Heidelberg, Germany
3
Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
Corresponding author: Send offprint request to: N.H. Youssef, cu090@frcu.eun.eg
Received:
18
August
1997
Accepted:
7
October
1997
A high resolution spectrum of a large - sunspot umbra is used for
identification of two bands and
of
the
-
system of the FeH molecule, in addition to the previously
identified bands
and
of the same system. The spectrum was
obtained with FTS of the McMath-Pierce Solar Telescope of NSO/NOAO at
Kitt Peak.
Key words: molecular data / Sun: atmosphere / Sun: sunspots
© European Southern Observatory (ESO), 1998