The ultraviolet spectrum of KX Trianguli Australis

Details The ultraviolet spectrum of KX Trianguli Australis The ultraviolet spectrum of KX Trianguli Australis

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...375..335f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 375, July 1, 1991, p. 335-341.

Astronomy and Astrophysics

Astrophysics

6

Symbiotic Stars, Ultraviolet Spectra, White Dwarf Stars, Electron Density (Concentration), Iron, Iue, Stellar Spectra, Subdwarf Stars

Scientific paper

Low-dispersion and high-dispersion IUE satellite observations of the symbiotic star KX TrA, carried out on May 7, 1990, are reported. The low-dispersion data show no significant changes from the observation data obtained a decade ago. Resonantly excited high-excitation Fe II emission lines are seen in the UV spectra of KX TrA, suggesting the existence of a very hot (greater than 60,000 K) subdwarf or white dwarf in the system. The S-type symbiotic KX TrA exhibits a UV spectrum that is nearly identical to that of the D-type symbiotic V1016 Cyg.

Affiliated with

Also associated with

No associations

Rating

The ultraviolet spectrum of KX Trianguli Australis 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 ultraviolet spectrum of KX Trianguli Australis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The ultraviolet spectrum of KX Trianguli Australis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-861101