The hydrogen-deficient irregular variable star V348 SGR

Details The hydrogen-deficient irregular variable star V348 SGR The hydrogen-deficient irregular variable star V348 SGR

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..363k&link_type=abstract

In ESA Fourth European IUE Conf. p 363-366 (SEE N84-35135 24-88)

Computer Science

1

Abundance, Hydrogen, Interstellar Extinction, Irregular Variable Stars, Nebulae, Variable Stars, Chromosphere, Iue, Stellar Composition, Stellar Spectra, Ultraviolet Spectroscopy

Scientific paper

The distribution of the reddening material around V 348 Sgr was studied using the IUE low resolution spectra. The nebula surrounding the star has a reddening of E(B-V) = 0.3 caused mainly by the foreground interstellar medium. The reddening in the chromosphere (CII emission line region) is E(B-V)=0.9. The star shows variable circumstellar reddening and extinction. The nebula appears to be carbon poor and nitrogen rich whereas earlier optical studies show that in the chromosphere the abundance of carbon, helium, and neon are enhanced and hydrogen is very deficient. Thus there seems to be chemical separation between the nebula and the star.

Affiliated with

Also associated with

No associations

Rating

The hydrogen-deficient irregular variable star V348 SGR 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 hydrogen-deficient irregular variable star V348 SGR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The hydrogen-deficient irregular variable star V348 SGR will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1705919