Computer Science
Scientific paper
Nov 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..547..255s&link_type=abstract
ATOMIC PROCESSES IN PLASMAS: Twelfth Topical Conference. AIP Conference Proceedings, Volume 547, pp. 255-264 (2000).
Computer Science
Atomic Processes And Interactions, Zeeman And Stark Effects, Line Shapes, Widths, And Shifts
Scientific paper
Magnetic white dwarfs possess strong magnetic fields which can vary in the wide range 100 T-105T. Atoms and molecules of their atmospheres which are exposed to such extreme fields severely change their electronic structure and properties. In order to understand the observed spectra of magnetic cosmic objects it is indispensable to perform detailed investigations on atoms in strong magnetic fields. As a recent example, we discuss the explanation of the absorption features of GD229 through the transitions of the Helium atom in a field of the order of 5.104 T. The complicated scenario of the ground state crossovers for multi-electron atoms in strong fields is outlined for the example of the carbon atom. .
No associations
LandOfFree
Magnetized atoms in star atmospheres 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 Magnetized atoms in star atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetized atoms in star atmospheres will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1147838