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Mass to line-strength relations from IUE spectra of early-type stars
An extensive survey of the 1200-1900 A region in OB type stellar spectraobtained from the IUE archives has been used to establish line-strengthversus spectral-type relationships. One hundred and sixty-threelow-resolution IUE spectra of 124 well-classified O3 to B5 stars wereexamined. Earlier results that the equivalent width of Si IV (1400 A)and C IV (1550 A) features are well correlated with optical spectraltype are confirmed. The equivalent width/spectral type/luminosity classrelations for these features are then established.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Pegasus |
| Ascensió Recta: | 22h08m45.79s |
| Declinació: | +34°30'15.8" |
| Magnitud Aparent: | 8.709 |
| Distancia: | 274.725 parsecs |
| Moviment propi RA: | -7.7 |
| Moviment propi Dec: | -7.8 |
| B-T magnitude: | 10.104 |
| V-T magnitude: | 8.825 |
Catàlegs i designacions:
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