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Issue A&A
Volume 369, Number 1, April I 2001
Page(s) 99 - 107
Section Formation, structure and evolution of stars
DOI http://dx.doi.org/10.1051/0004-6361:20010031



A&A 369, 99-107 (2001)
DOI: 10.1051/0004-6361:20010031

A representative sample of Be stars

IV. Infrared photometry and the continuum excess
Lee Howells, I. A. Steele, John M. Porter and J. Etherton

Astrophysics Research Institute, Liverpool John Moores University, Egerton Wharf, Birkenhead CH41 1LD, UK

(Received 1 September 2000 / Accepted 22 December 2000)

Abstract
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity classes III-V. We describe a new method of reduction, enabling separation of interstellar reddening and circumstellar excess. Using this technique we find that the disc emission makes a maximum contribution to the optical (B-V) colour of a few tenths of a magnitude. We find strong correlations between a range of emission lines (H$\alpha$, Br$\gamma$, Br11, and Br18) from the Be stars' discs, and the circumstellar continuum excesses. We also find that stellar rotation and disc excess are correlated.


Key words: stars: emission-line, Be -- circumstellar matter -- stars: rotation -- techniques: photometric -- methods: data analysis

Offprint request: Lee Howells, lxh@astro.livjm.ac.uk

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© ESO 2001


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