The celebrated Herbig AE star, AB Aur. I - Investigation of the emission-line variability at 0.37-0.88 micron

Details The celebrated Herbig AE star, AB Aur. I - Investigation of the emission-line variability at 0.37-0.88 micron The celebrated Herbig AE star, AB Aur. I - Investigation of the emission-line variability at 0.37-0.88 micron

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..459s&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Dec. 1987, p. 459-470. In Russian.

Astronomy and Astrophysics

Astronomy

2

A Stars, Emission Spectra, H Lines, Infrared Spectra, Spectral Energy Distribution, Spectral Line Width, Electrophotometry, H Alpha Line, H Beta Line, H Gamma Line

Scientific paper

The variability of AB Aur emission line profiles, equivalent widths and relative intensity of Hα, Hβ, Hγ have been observed on the photoelectric scanner. The AB Aur variability nature of emission lines made it possible to assume that the "deep chromosphere" is not a centre-symmetrical or axisymmetrical formation but is a conglomerate of gas condensations with different density and speed.

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