Distribution of absolute energy of bright Be stars in Pleiades

Details Distribution of absolute energy of bright Be stars in Pleiades Distribution of absolute energy of bright Be stars in Pleiades

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.105..323g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 105, no. 2, Oct. 1984, p. 323-330.

Astronomy and Astrophysics

Astrophysics

9

B Stars, Pleiades Cluster, Spectral Energy Distribution, Stellar Spectra, Variable Stars, Balmer Series, Continuous Spectra, Interstellar Extinction, Late Stars, Stellar Temperature

Scientific paper

The authors present newly measured energy distributions from λλ3200 - 7500 Å of five late-type Be stars in the Pleiades cluster for search of peculiarities of Be stars continuum energy distributions. Empirical effective temperatures of Be stars have been derived by comparing observed and computed fluxes in the visible region. The variation of the flux in the Balmer continuum region of Pleione (28 Tau) has been discussed.

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