Abstract
We present preliminary results of observations of IR [FeII] lines in the direction of SNR. In all the spectra the [FeII] 1.644μm line is by far the brightest feature in the observed spectrum and its intensity is comparable to that of Hß. Reddening and electron density are estimated for the best measured objects. Implications on the Fe abundance are briefly discussed.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Leibowitz, E.M., Danziger, I.J.: 1983, M.N.R.A.S., 204, 273.
Danziger, I.J., Leibowitz, E.M.: 1985, M.N.R.A.S., 216, 365.
McKee, C.F., Chernoff, D.F., Hollenbach, D.J.: 1984, Galactic and Extragalactic IR Spectroscopy, Astrophysics and Space Science Library, 108, 103, Kessler, M.F. and Phillips, J.P. eds. (D. Reidel Publ. Co.).
Moorwood, A.F.M. et al.: 1986, The Messenger, 44, 19.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1988 D. Reidel Publishing Company
About this paper
Cite this paper
Oliva, E., Moorwood, A.F.M., Danziger, I.J. (1988). Infrared Lines of [FeII] from Supernova Remnants. In: Viotti, R., Vittone, A., Friedjung, M. (eds) Physics of Formation of FeII Lines Outside LTE. Astrophysics and Space Science Library, vol 138. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4023-9_22
Download citation
DOI: https://doi.org/10.1007/978-94-009-4023-9_22
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8285-3
Online ISBN: 978-94-009-4023-9
eBook Packages: Springer Book Archive