Integrated UV magnitudes of the Large Magellanic Cloud associations

Details Integrated UV magnitudes of the Large Magellanic Cloud associations Integrated UV magnitudes of the Large Magellanic Cloud associations

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...72..249v&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 72, no. 2, Feb. 1988, p. 249-257.

Statistics

Computation

6

Galactic Clusters, Light Scattering, Magellanic Clouds, Star Formation, Ultraviolet Astronomy, Ultraviolet Spectrophotometers, Angular Resolution, Computational Astrophysics, Error Analysis, Least Squares Method, Skylab Program

Scientific paper

UV photographs (2600 Å, 350 Å passband) of the Large Magellanic Cloud have been obtained by the S183 experiment during a Skylab mission. The background is estimated and a method for deriving the integrated fluxes is presented. The author gives the integrated magnitudes of about 50 associations and isocontours of their intensities. He presents also B and V integrated magnitudes of 13 associations.

Affiliated with

Also associated with

No associations

Rating

Integrated UV magnitudes of the Large Magellanic Cloud associations 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 Integrated UV magnitudes of the Large Magellanic Cloud associations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Integrated UV magnitudes of the Large Magellanic Cloud associations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1224592