Abstract
Low frequency recombination lines will be defined for the purpose of this paper, to be those transitions with frequencies significantly less than 1 GHz. Most radio recombination line observations have been carried out at high frequencies, as not only can higher angular resolution be obtained, but also the signal-to-noise ratio is higher for small diameter, high emission measure objects and there are less problems with the optical depth of the free-free emission.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Batty, M.J., (1974), Mon.Not.R.astr.Soc., 168, 37 P.
Bignell, R.C., (1973), Astrophys.J., 186, 889.
Brocklehurst, M. and Seaton, M.J., (1972), Mon.Not.R. astr.Soc. 157, 179.
Brown, R.L. and Balick, B. (1973), Astrophys.J. 185, 843.
Casse, J.L. and Shaver, P.A., (1977), Astr on.Astrophys. 61, 805.
Cesarsky, D.A. and Cesarsky, C.J., (1973a), Astrophys.J. 183, L143.
Cesarsky, D.A. and Cesarsky, C.J., (1973b), Astrophys.J. 184, 83.
Chaisson, E.J., (1974), Astrophys.J., 189, 69.
Churchwell, E., (1971), Astron. Astrophys. 15, 90.
Churchwell, E., (. 1975 ), Proceedings of Mittelberg Syinposium, Lecture Notes in Physics 4 - 2, Springer-Verlag, Berlin
Downes, D. and Wilson, T.L. (1974), Astron.Astrophys. 34, 133.
Dupree, A.K. and Goldberg, L., (1969), Astrophys.J. 158, L49.
Dyson, J.E., (1969), Astrophys.Sp.Sci., 4, 401.
Gordon, K.J., Gordon, C.P. and Lockman, F.J. (1974), Astrophys.J. 192, 337.
Gordon, M.A. and Cato, T., (1972), Astrophys.J. 176, 587.
Gordon, M.A. and Gottesman, S.T., (1971), Astrophys.J. 168, 361.
Hart, L., Ediss, G.A. and Pedlar, A. (1980) (in preparation).
Hart, L. and Pedlar, A., (1976), Mon.Not.R.astr.Soc. 176, 547.
Jones, B.B. and Finley, E.A. (1974), Australian J.Phys.27, 687.
Lang, K.R. and Willson, R.F., (1978), Mon.Not.R.astr.Soc. 183, 5 P.
Lockman, F.J., (1976), Astrophys.J. 209, 429.
Lockman, F.J. and Gordon, M.A. (1973), Astrophys.J. 182, 25.
Matthews, H.E., Davies, R.D. and Fedlar, A., (1973), Mon.Not.R.astr.Soc. 165, 173.
Mezger, P.G. and Henderson, A.P., (1967), Astrophys.J. 147, 471.
Pankonin, V., (1975), Astron.Astrophys. 38, 445.
Parrish, A., Conklin, E.K. and Pankonin, V. (1977), Astron. Astrophys., 58, 319.
ParrisE, A., Pankonin, V., Heiles, C.E., Rankin, J.M. and Terzian, Y., (1972), Astrophys. J., 178, 673.
Parrish, A., and Pankonin, V., (1975), Astrophys.J., 198, 349.
Pedlar, A. (1980) (Submitted to Mon.Not.R.astr.Soc.)
Pedlar, A. and Davies, R.D., (1971), Nature 231, 49.
Pedlar, A. and Davies, R.D., (1972), Mon.Not.R.astr.Soc., 159, 129.
Pedlar, A., Davies, R.D., Hart, L. and Shaver, P.A., (1978), Mon.Not. R.astr. Soc., 182, 473.
Pedlar, A. and Matthews, H.E. (1973), Mon.Not.R.astr.Soc., 165, 381.
Penfield, H., Palmer, P. and Zuckerman, B. (1967), Astrophys J. 148, L25.
Shaver, P.A., (1975), Pramina, 5, 1.
Shaver, P.A., (1976), Astron.Astrophys., 49, 1.
Shaver, P.A., (1976), Astron.Astrophys., 59, L31.
Shaver, P.A., Pedlar, A.,Davies, R.D. (1976), Mon.Not.R.astr.Soc., 177, 45.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1980 D. Reidel Publishing Company
About this paper
Cite this paper
Pedlar, A., Davies, R.D. (1980). Low Frequency Recombination Lines. In: Shaver, P.A. (eds) Radio Recombination Lines. Astrophysics and Space Science Library, vol 80. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9024-1_16
Download citation
DOI: https://doi.org/10.1007/978-94-009-9024-1_16
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-9026-5
Online ISBN: 978-94-009-9024-1
eBook Packages: Springer Book Archive