Titlebook: B[e] Stars; Anne Marie Hubert,Carlos Jaschek Book 1998 Springer Science+Business Media B.V. 1998 Galaxy.LOPES.galaxies.interferometry.phot

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Automated Staining: Dako Perspective,ins the .. and .. magnitudes measured for each Tycho observation of the known variable stars. In the present paper, these measurements are corrected for the bias described in ESA SP-1200, Vol. 4, chapter 9 (pg 133).

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Tycho Photometry of some B[e] Starsins the .. and .. magnitudes measured for each Tycho observation of the known variable stars. In the present paper, these measurements are corrected for the bias described in ESA SP-1200, Vol. 4, chapter 9 (pg 133).

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Search for B[e] Stars in Young Open Clustersclude that none of the ~ 260 relatively young early type stars can be identified as such. We propose that either the B[e] characteristic is not present in young stars or that due to the close proximity of other hot stars the circumstellar material cannot hold sufficient amounts of material to show t

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Tycho Photometry of some B[e] Starshan .. =11.5 mag (ESA 1997, ESA SP-1200) . These two filters are roughly centered on the B and V Johnson filters. A simple linear transformation exists between Tycho .. and . magnitudes and B and V magnitudes in the Johnson photometric system (see ESA 1997) . The Tycho Epoch Photometry Annex A conta