Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.249..257c&link_type=abstract
Astrophysics and Space Science, Volume 249, Issue 2, pp.257-268
Astronomy and Astrophysics
Astrophysics
Scientific paper
We use statistical data giving the number of stars formed as a function of the age, assigned using the observed deterministic relation between chromospheric activity and age, to show that the temporal behaviour of star formation in the solar neighbourhood must have been chaotic during time intervals of less than 1 Gyr. We also offer evidence that systems of gas and stars typified by that in the solar vicinity show behaviour analogous to that of the logistic map.
Beckman John E.
Casuso Emilio
No associations
LandOfFree
Chaotic Behaviour of the Temporal Evolution of Star Formation Rate in the Solar Neighborhood does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Chaotic Behaviour of the Temporal Evolution of Star Formation Rate in the Solar Neighborhood, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chaotic Behaviour of the Temporal Evolution of Star Formation Rate in the Solar Neighborhood will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1316618