Abstract
Microphotometric tracings of the spectrograms of carbon stars with the dispersion of 8A/mm from the spectral region λ 7800 to λ 8800 are discussed in connection with the identification of 12CN, 13CN, HCN, [CI] λ8727, and telluric H2O lines. The microphotometric tracing of the same region of an M-type star μ Cep seems very helpful for the identification of telluric H2O lines.
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
Preview
Unable to display preview. Download preview PDF.
References
Davis,D.N.: 1947, Astrophys.J. 106, 28.
Fujita,Y.:1973, Proc. Japan Acad. 49, 530.
Fujita,Y.:1977, Journ. Roy. Astron. Soc. Canada, 71, 115.
Fujita,Y.: 1978, Proc. Japan Acad. 54,Ser.B;, 207.
Fujita,Y.:1980, Proc. Japan Acad. 56,Ser.B, 399.
Fujita,Y.:1981, Proc. Japan Acad. 57,Ser.B, 169.
Fujita,Y.:1983, Proc. Japan Acad. 59,Ser.B, 145.
Lambert,D.L. and Swings,J.P.:1967, Solar Phys. 2, 34.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1985 D. Reidel Publishing Company
About this paper
Cite this paper
Fujita, Y. (1985). Identification of Photographic Infrared Spectral Region in Carbon Stars. In: Jaschek, M., Keenan, P.C. (eds) Cool Stars with Excesses of Heavy Elements. Astrophysics and Space Science Library, vol 114. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5325-3_5
Download citation
DOI: https://doi.org/10.1007/978-94-009-5325-3_5
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8851-0
Online ISBN: 978-94-009-5325-3
eBook Packages: Springer Book Archive