Other
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..133f&link_type=abstract
In ESA Fourth European IUE Conf. p 133-137 (SEE N84-35135 24-88)
Other
1
A Stars, Absorption Spectra, Interstellar Extinction, Ultraviolet Spectra, Interstellar Chemistry, Iue, Magnesium
Scientific paper
The interstellar medium in the direction of four A-stars that are fast rotators, in the range 1250 to 1800 A, and 7 fast rotators and 2 low rotators in the range 2000 to 3000 A was studied by IUE. Interstellar Mg II absorption is observed, centered or not in the stellar line cores. Other interstellar lines probably present are Fe II, A1 II, Si II, C II and S II. The A-type stars that rotate slowly may also be useful to determine Mg II interstellar contributions, when the theoretical stellar Mg II line profile is known. Preliminary widths of these interstellar lines are deduced from the observations.
No associations
LandOfFree
The interstellar absorption in the direction of some nearby A stars 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 The interstellar absorption in the direction of some nearby A stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The interstellar absorption in the direction of some nearby A stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1705628