Ultraviolet observations of Mira Ceti

Details Ultraviolet observations of Mira Ceti Ultraviolet observations of Mira Ceti

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157..233c&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

4

Binary Stars, Iue, Mira Variables, Stellar Mass Accretion, Ultraviolet Astronomy, Variable Stars, Absorption Spectra, Continuous Spectra, Cosmic Dust, Disks (Shapes), Emission Spectra, Giant Stars, Lyman Alpha Radiation, Stellar Mass Ejection, White Dwarf Stars

Scientific paper

International Ultraviolet Explorer observations of Mira Ceti show a wealth of emission lines, a continuum gradually increasing to long wavelengths and a number of absorption features due to Fe II, Mg II and perhaps Fe I and CO. These spectral components exhibit some variability and can be explained with a model of accretion into a disk around Mira B (a white dwarf) of material from Mira A (M6IIIe).

Affiliated with

Also associated with

No associations

Rating

Ultraviolet observations of Mira Ceti 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 Ultraviolet observations of Mira Ceti, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet observations of Mira Ceti will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1698317