Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· References in the article
· Citations to the Article (9) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Isotopic abundance in the CN coma of comets: Ten years of measurements
Authors:
Schulz, R.; Jehin, E.; Manfroid, J.; Hutsemékers, D.; Arpigny, C.; Cochran, A.; Zucconi, J.-M.; Stüwe, J. A.
Affiliation:
AA(Research and Scientific Support Department, ESA, Postbus 299, 2200 AG Noordwijk, The Netherlands), AB(Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 août 17, 4000 Liège, Belgium), AC(Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 août 17, 4000 Liège, Belgium), AD(Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 août 17, 4000 Liège, Belgium), AE(Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 août 17, 4000 Liège, Belgium), AF(Department of Astronomy and McDonald Observatory, University of Texas, Austin, TX 1400, USA), AG(Observatoire de Besançon, F25010 Besançon Cedex, France), AH(Leiden Observatory, NL-2300 RA Leiden, The Netherlands)
Publication:
Planetary and Space Science, Volume 56, Issue 13, p. 1713-1718. (P&SS Homepage)
Publication Date:
11/2008
Origin:
ELSEVIER
DOI:
10.1016/j.pss.2008.08.001
Bibliographic Code:
2008P&SS...56.1713S

Abstract

Over the past 10 years the isotopic ratios of carbon (12C/13C) and nitrogen (14N/15N) have been determined for a dozen comets, bright enough to allow obtaining the required measurements from the ground. The ratios were derived from high-resolution spectra of the CN coma measured in the B2+-X2+ (0, 0) emission band around 387 nm. The observed comets belong to different dynamical classes, including dynamically new as well as long- and short-period comets from the Halley- and Jupiter-family. In some cases the comets could be observed at various heliocentric distances. All values determined for the carbon and nitrogen isotopic ratios were consistent within the error margin irrespective of the type of comet or the heliocentric distance at which it was observed. Our investigations resulted in average ratios of 12C/13C=91±21 and nitrogen 14N/15N=141±29. Whilst the value for the carbon isotopic ratio is in good agreement with the solar and terrestrial value of 89, the nitrogen isotopic ratio is very different from the telluric value of 272.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

  New!

Find Similar Abstracts:

Use: Authors
Title
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints