SK-67/111 and R 50, two Magellanic Cloud emission line stars

Details SK-67/111 and R 50, two Magellanic Cloud emission line stars SK-67/111 and R 50, two Magellanic Cloud emission line stars

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..277z&link_type=abstract

In ESA 3rd European IUE Conf. p 277-279 (SEE N83-11889 02-88)

Physics

1

Emission Spectra, Hot Stars, Magellanic Clouds, Stellar Mass Ejection, H Alpha Line, Iue, Late Stars, Resonance Lines, Stellar Envelopes

Scientific paper

The SK-67/111 (05f) of the large Magellanic Cloud (LMC) and the peculiar emission line star R 50 of the small cloud were observed by IUE and by telescope. From the Si IV resonance doublet a mass loss rate of 0.000005 M/yr was obtained for SK-67/111, in agreement with calculations based on the H alpha emission intensity. No significant difference is found for this LMC star with the mass loss rate of corresponding galactic stars. Observations of R 50 show that it is a late B type star surrounded by a cool dense envelope. Its mass loss rate is on the order of 0.00005 M/yr.

Affiliated with

Also associated with

No associations

Rating

SK-67/111 and R 50, two Magellanic Cloud emission line 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 SK-67/111 and R 50, two Magellanic Cloud emission line stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SK-67/111 and R 50, two Magellanic Cloud emission line stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1353419