FeII and MgII in the nearby interstellar medium

Details FeII and MgII in the nearby interstellar medium FeII and MgII in the nearby interstellar medium

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2345...71d&link_type=abstract

In NASA. Goddard Space Flight Center Local Interstellar Medium, No. 81 p 71-74 (SEE N85-15539 06-90)

Physics

2

Interstellar Matter, Ions, Iron, Iue, Magnesium, Balloon-Borne Instruments, Brightness Distribution, Spectral Resolution, Stellar Rotation

Scientific paper

UV spectra with 15 km sec-1 resolution of bright stars have been searched for Fe II and Mg II interstellar lines. The authors present equivalent widths of absorption for 8 stars and find average line-of-sight densities n(Fe II) = 4×10-8 and n(Mg II) = 2×10-7cm-3. This represents approximately n(H) = 0.03 cm-3.

Affiliated with

Also associated with

No associations

Rating

FeII and MgII in the nearby interstellar medium 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 FeII and MgII in the nearby interstellar medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and FeII and MgII in the nearby interstellar medium will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1755753