Mira B

Details Mira B Mira B

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.199.1113s&link_type=abstract

(ESA, Villafranca Satellite Tracking Station, Madrid, Spain). Royal Astronomical Society, Monthly Notices, vol. 199, June 1982,

Astronomy and Astrophysics

Astronomy

9

Absorption Spectra, Companion Stars, Emission Spectra, Mira Variables, Stellar Spectrophotometry, Ultraviolet Spectra, Variable Stars, Abundance, B Stars, High Resolution, Iue, M Stars, Periodic Variations, Spectral Line Width, Spectral Resolution, Stellar Envelopes, Ultraviolet Astronomy

Scientific paper

A high resolution IUE spectrum of Mira taken at the time of the 1980
maximum shows sharp emission features from the M star and broad ones
attributable to a large volume of gas around the hot companion. Some
information on the emission from the vicinity of Mira B is available
from line widths and ratios.

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