Journal
ASTRONOMY & ASTROPHYSICS
Volume 469, Issue 1, Pages 201-206Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20077077
Keywords
ISM : clouds; ISM : molecules
Categories
Ask authors/readers for more resources
We have used the ionisation equilibrium equation to derive the electron density in interstellar clouds in the direction of 13 stars. A linear relation was found that allows determination of the electron density from the Mg I and MgII column densities in diffuse clouds. The comparison of a normalised equivalent width of 12 DIBs with the electron density shows that the DIBs equivalent width do not change with electron density varying in the range ne = 0.01 divided by 2.5 cm(-3). Therefore the DIBs carriers (1) can be observed only in one ionisation stage, or (2) the DIBs are arising in cloud regions (eg. cores or cloud coronas) for which we cannot determine the electron density.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available