The visible spectra of three B stars - Pi Cet, 36 Lyn, and 134 Tau

Bibcode
1981Ap&SS..80..425C
DOI
10.1007/BF00652941
Crivellari, L.; Flora, U.; Mercanti, M.; Morossi, C.; Rusconi, L.; Sedmak, G.
Referencia bibliográfica

Astrophysics and Space Science, vol. 80, no. 2, Dec. 1981, p. 425-436. Research supported by the Consiglio Nazionale delle Richerche.

Fecha de publicación:
12
1981
Revista
Astrophysics and Space Science
Número de autores
6
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
An identification list is presented for the visible spectra of Pi Cet (B7 V), 36 Lyn (B8 IIIp), and 134 Tau (B9 IV). Equivalent widths are measured on medium dispersion plates of 7.0 and 12.4 A/mm, and the photographic plates are digitized using a PDS 1010A microdensiometer. The effective temperature and gravity of the three stars are estimated, and the spectroscopic data are compared with values from theoretical models showing good internal consistency.
Tipo
Con árbitro
Estrellas B

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