Comparison of the spectrophotometric data of two FeII emission line stars

Details Comparison of the spectrophotometric data of two FeII emission line stars Comparison of the spectrophotometric data of two FeII emission line stars

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26as...43..111m&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 43, Jan. 1981, p. 111-119.

Astronomy and Astrophysics

Astrophysics

6

Emission Spectra, Iron, Line Spectra, Stellar Spectra, Stellar Spectrophotometry, Fine Structure, Radial Velocity, Spectral Line Width, Tables (Data)

Scientific paper

Line identifications have been made from 74-52 and 20 A/mm plates of the SMC star R50 and LMC star R82, whose spectra are similar. Both stars show P Cygni profiles for the Balmer lines. In the case of the FeII lines, P Cygni profiles are clearly visible for R82 and possibly present for R50. Identifications, radial velocities, equivalent widths, peak intensities above the continuum as well as half intensity widths are given for all lines. Radial velocity variations are suggested for both stars.

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