V AND i IN ROTATING STARS FROM COPERNICUS UV DATA

V AND i IN ROTATING STARS FROM COPERNICUS UV DATA

Measurements of line widths are presented in the far UV and visual for samples of high-and lowrotation early-type stars. By means of calculations previously reported, the ratio of these values, and values of V sin i enable a determination of V and i. The results are discussed briefly.

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Bibliographische Detailangaben
Veröffentlicht in:Publications of the Astronomical Society of the Pacific 1977-02, Vol.89 (527), p.19-22
Hauptverfasser: HUTCHINGS, J. B., STOECKLEY, T. R.
Format: Artikel
Sprache:eng
Schlagworte:
Data lines
Fall lines
Preprints
Rotational spectra
Sine function
Stars
Stellar rotation
Stellar spectra
Stellar spectral lines
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Beschreibung
Zusammenfassung:Measurements of line widths are presented in the far UV and visual for samples of high-and lowrotation early-type stars. By means of calculations previously reported, the ratio of these values, and values of V sin i enable a determination of V and i. The results are discussed briefly.
ISSN:0004-6280
1538-3873
DOI:10.1086/130062