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The flux of interstellar particles detected in the Solar System

Published online by Cambridge University Press:  01 February 2008

Mária Hajduková Jr.
Mária Hajduková Jr.*
Affiliation:
Astronomical Institute of the SlovakAcademy of SciencesDübravská cesta 9, 845 05 Bratislava, The Slovak Republic email: [email protected]
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Abstract

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The present work shows the proportion of interstellar meteors from different mass ranges (exceeding 20 orders of mass scale) detected by various observational techniques. Having analysed the IAU Meteor Data Center, we find that the mass index of interstellar particles continuously increases towards higher masses, but there is a significant change between 10−10 − 10−11 kg. This break is possibly caused by different physical processes leading to different populations of interstellar particles and might be connected with their origin.

Keywords

Meteorsmeteoroidsinterplanetary medium
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S251: Organic Matter in Space , February 2008 , pp. 345 - 346
Copyright
Copyright © International Astronomical Union 2008

References

Divine, N., Grün, E., & Staubach, P. 1993, in: Flury, W., Darmstadt, (eds.), Proceeding of the First European Conference on Space Debris, ESA SD - 01, p. 245Google Scholar
Fechtig, H. 1976, in: Hemenvay, C. L., Millman, P. M. and Cook, A. F. (eds.), Evolutionary and Physical Properties of Meteoroids, NASA SP, 319, p. 218Google Scholar
Hajduková, M. Jr. 1994, A&A, 288, 330Google Scholar
Hajduková, M. Jr. 2008, Earth, Moon, Planets, 102, 67CrossRefGoogle Scholar
Hajduková, M. Jr. & Hajduk, A. 2006, Contri. Astron. Obs. Skalnaté Pleso, 36, 15Google Scholar
Hawkes, R. L. & Woodworth, S. C. 1997a, J. R. Astron. Soc. Can., 91, 68Google Scholar
Hawkes, R. L. & Woodworth, S. C. 1997b, J. R. Astron. Soc. Can., 91, 218Google Scholar
Lindblad, B. A., Neslušan, L., Porubčan, V., & Svoreň, J. 2005, Earth, Moon, Planets, 93, 249CrossRefGoogle Scholar
Mathews, J. D. et al. 1999, in: Baggaley, W. J. and Porubčan, V. (eds.), Meteoroids 1998, (Slovak Academy of Sciences, Bratislava), p. 79Google Scholar
Weryk, R. J. & Brown, P. 2005, Earth, Moon, Planets 95, 221CrossRefGoogle Scholar