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FIR and sub-mm line observations of AGB and post-AGB nebulae
Published online by Cambridge University Press: 21 October 2010
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The existing information on asymptotic giant branch (AGB) and post-AGB objects from FIR and submm spectroscopy is still scarce. Observations from the ground are often very difficult to calibrate and show low S/N ratios. However, we expect to obtain in the near future an impressive amount of high-quality data, from the Herschel space telescope. ALMA is also expected to provide high-quality maps of submm lines.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 550 - 551
- Copyright
- Copyright © International Astronomical Union 2010
References
Bujarrabal, V., Castro-Carrizo, A., Alcolea, J., & Sánchez Contreras, C. 2001, A&A 377, 868Google Scholar
Groenewegen, M. A. T.; van der Veen, W. E. C. J., & Matthews, H. E. 1998, A&A 338, 491Google Scholar
Sánchez Contreras, C., Bujarrabal, V., & Castro-Carrizo, A. 2004, ApJ 617, 1142CrossRefGoogle Scholar
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