Line profile variations in M giants - Clues to mass-loss and chromospheric heating mechanisms

Abstract

view Abstract Citations (8) References (45) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Line Profile Variations in M Giants: Clues to Mass-Loss and Chromospheric Heating Mechanisms Judge, P. G. ; Luttermoser, D. G. ; Neff, D. H. ; Cuntz, M. ; Stencel, R. E. Abstract Analysis is presented of time-series, high dispersion spectra of the Mg II, k, Ca II H, and K lines of the semiregular giants Rho Per (M4 II-III, periodicity of about 50 days), R Lyr (M5 III, period of about 46 days), and g Her (M6 III, period of about 90 days). The fine error sensor on the IUE satellite and ground based UBV photometry was used to relate line profile variations to photospheric variations. The above mentioned stars were selected to study the relative importance of convective motions and global stellar pulsations in determining the structure of the outer atmospheres. Small amplitude changes, but substantial changes in the profiles of Mg II and Ca II lines were detected. It is contended that the observed variability is due to changes in chromospheric conditions and not variations within the circumstellar shell. The picture of a steady state chromosphere, which is modulated on long time scales, is corroborated by these observations. Localized heating is found in g Her. Publication: The Astronomical Journal Pub Date: May 1993 DOI: 10.1086/116573 Bibcode: 1993AJ....105.1973J Keywords: Giant Stars; M Stars; Spectral Line Width; Stellar Mass Ejection; Stellar Motions; Stellar Oscillations; Astronomical Photometry; Atmospheric Heating; Chromosphere; Data Reduction; Iue; Stellar Envelopes; Ubv Spectra; Astrophysics; STARS: GIANTS; STARS: MASS-LOSS; STARS: CHROMOSPHERES full text sources ADS | data products SIMBAD (6) MAST (1) INES (1)